The galaxy presents a predominantly smooth morphology, with a central bulge that exhibits a bright, concentrated luminosity. The overall color index suggests a population of older stars, contributing to its yellowish-white hue. There is some indication of a faint disk-like structure surrounding the bulge, though it lacks distinct spiral arms or well-defined features. The outer regions appear diffuse and gradually fade into the background sky, implying a decreasing stellar density with increasing radius from the galaxy's center. Evidence of any significant tidal interactions or ongoing merging events is generally absent, although there is some slight asymmetry, suggesting minor disturbances or past interactions could have occurred. Overall, the galaxy seems like a relatively evolved system.
