The galaxy presents an elliptical morphology, though with a noticeable degree of disk-like structuring. The central region exhibits a smooth, concentrated bulge that displays a reddish-yellow hue, suggestive of an older stellar population. The outer regions of the galaxy show a transition to a bluer color, indicative of younger, hotter stars and potential star-forming regions. There's a slight indication of dust lanes or other features disrupting the smoothness, particularly in the equatorial regions. The galaxy appears to be in a relatively isolated state, though there are possible signs of a minor tidal disturbance. The overall form appears more elongated and cigar-shaped, rather than perfectly round.
