The galaxy presents a generally smooth morphology, with a centrally concentrated light profile. It is primarily elliptical in shape, though not perfectly spherical. There is a slight elongation, appearing more "in-between" round and cigar-shaped. The central region exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color shifts subtly towards the red end of the spectrum. There is no clear evidence of spiral arm structure or significant dust lanes. There appears to be only very minor disturbance of the galaxy, suggesting it is fairly stable at this point in time. The overall structure indicates a system that has likely undergone significant merging events in its past, resulting in its current morphology.
