The galaxy presents as a relatively smooth, centrally concentrated object. It is elliptical in shape, displaying a somewhat elongated morphology. A bright, yellowish core is dominant, suggesting an older stellar population residing in the nucleus. The outer regions exhibit a bluer hue, which could be indicative of ongoing, albeit low, star formation or the presence of a younger stellar population within the galaxy's disk. There is no obvious spiral arm structure. No signs of a major merger are present. Minor asymmetric dust lanes may be present, suggesting a potential minor disturbance. The overall appearance indicates a galaxy that is transitioning to a redder color with a slightly flattened spheroidal shape.
