The galaxy presents as a relatively smooth, elliptical form. There is a concentrated central bulge with a yellowish-orange hue, suggestive of an older stellar population. The surrounding galactic disk exhibits a bluer tint, hinting at the presence of some younger stars or regions of ongoing star formation, but it is a subtle effect. The overall shape is oblong, deviating from a perfect circle, with a suggestion of a slight tidal disturbance or minor interaction visible in the disk. It does not appear to be undergoing a major merger or exhibit significant tidal tails.
