The galaxy presents as an elongated, elliptical form. Its central region appears luminous and displays a yellowish hue, suggestive of an older stellar population. The outer regions exhibit a gradual decline in brightness, fading into the background. There is no apparent structure indicative of spiral arms or prominent dust lanes. The overall morphology implies a relatively smooth distribution of light, consistent with an early-type galaxy. Faint blue colors around the disk could suggest recent star formation. Close inspection does not reveal any obvious signs of ongoing major mergers or tidal disturbances.
