The galaxy presents as an interacting system, exhibiting morphological disturbances suggestive of tidal forces. Two primary components are discernible: a larger, more luminous central body, and a smaller, less luminous companion. 

The larger component appears roughly elliptical in overall shape, although its morphology is not perfectly smooth; there is an indication of disruption in its outer regions. The light distribution is concentrated towards the core, fading gradually towards the edges.

The smaller companion is more elongated and cigar-shaped, indicating a possible disk-like structure viewed at an angle or significant tidal deformation. Its light distribution is less centrally concentrated compared to the primary galaxy.

A faint bridge of light can be seen connecting the two galaxies, suggesting gravitational interaction. The overall color profile indicates a mixture of stellar populations. The primary galaxy exhibits a yellowish hue, which can potentially indicate the presence of an older, redder stellar population. The companion galaxy may have bluer regions, possibly signaling more recent star formation triggered by the interaction.
