The galaxy presents as a luminous, elliptical morphology, with an overall smooth and concentrated structure. It exhibits a distinct yellow-orange color profile, suggesting a stellar population dominated by older, evolved stars. The isophotes appear to be generally regular and concentric, although there is a slight elongation visible, indicating a deviation from perfect circularity. There is no clear evidence of spiral arms or prominent dust lanes. Faint outer regions suggest the presence of an extended halo, but the contrast is low. There are very minor apparent disturbances in the galaxy's shape which could be evidence of a small minor merger. The lack of visible blue light suggests a relatively low ongoing star formation rate.
