The galaxy appears to be a relatively bright, early-type system, exhibiting a smooth, elliptical morphology. It shows a centrally concentrated luminosity profile, suggestive of a large stellar bulge. There is a noticeable lack of prominent spiral arms or dust lanes, and the galaxy displays a fairly round shape, with a slight elongation that is close to circular. The color is relatively uniform across the galaxy, with a yellowish-red hue indicative of an older stellar population with minimal ongoing star formation. Subtle disturbances may be present, indicating a possible history of minor interactions, although the overall structure appears largely undisturbed.
