The galaxy presents a primarily smooth, elliptical morphology. The central bulge exhibits a concentrated, bright, yellowish-white hue, suggesting a population of older stars. There is an apparent disk structure exhibiting a slightly bluer tint, this indicates more recent star formation within that region. There is no strong evidence of spiral arm structure; however, subtle irregularities and minor disturbances can be seen, possibly indicative of a minor merging event. The apparent size of the galaxy suggests a large physical scale.
