The galaxy presents as a roughly elliptical object. A bright, concentrated central bulge dominates the morphology. The bulge exhibits a yellow-white color, suggesting a population of older stars. Fainter, diffuse arms extend outwards from the bulge. These arms exhibit a bluer tint, potentially indicative of ongoing star formation. The galaxy appears to be relatively isolated. There is no immediately obvious evidence of significant tidal interactions or a major merger event. There may be a slight asymmetry or minor disturbances in the outer regions, possibly related to minor interactions or internal dynamics. The overall morphology suggests that the galaxy may be an early-type spiral galaxy.
