The galaxy presents as an interacting system, likely a merger in progress. One component is a relatively bright, compact, and smooth spheroid. This spheroid appears to be at the earlier stages of the collision. The secondary component is more diffuse and elongated in form, exhibiting a yellowish hue. The observed color suggests an older stellar population or significant dust obscuration. There is evidence of a tidal tail or bridge of material connecting the two components, indicating gravitational interaction between the two. The merging process appears to be inducing star formation, most notably in the diffuse component. The system's morphology is irregular, deviating significantly from a standard spiral or elliptical form, further supporting its classification as a merger. There appears to be some distortion happening to the shape of both galaxies.
