The galaxy presents as a relatively smooth, elongated structure, exhibiting a possible disk-like component or disturbed morphology. One end displays a brighter, more concentrated core region characterized by a reddish hue. This suggests the presence of an older stellar population or significant dust obscuration within the core. Emanating from this core is a less defined, extended plume with a yellowish color, potentially indicating a more dispersed distribution of stars or a region of ongoing star formation. The overall shape deviates from a perfectly elliptical form, hinting at possible tidal interactions or internal dynamical processes. The light distribution suggests that the galaxy is neither a perfectly spherical elliptical nor a well-defined spiral, falling somewhere in between or exhibiting a disrupted structure.
