The galaxy presents as a relatively compact and centrally concentrated object. Its morphology appears to be generally smooth with an elliptical-like profile, lacking any obvious spiral arm structure. The light distribution is not perfectly symmetrical, but it displays a near regular shape with hints of elongation. There appears to be a slight color gradient, with the central region exhibiting a subtly yellowish-white hue, indicative of an older stellar population. This color shifts to a slightly bluer tone in the outer regions. Overall, the galaxy exhibits characteristics suggestive of a quiescent system dominated by older stars and possessing a moderate stellar mass.
