The galaxy presents a somewhat elliptical morphology, appearing neither perfectly spherical nor highly elongated. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus or a dense stellar population. There appears to be a slight asymmetry in the outer regions, possibly indicating a minor interaction or past merger event. Evidence for a disk-like structure exists but is not prominent. Color gradients suggest varying stellar populations, with the central region being a generally redder color, potentially indicating older stars or a higher dust content. The outer regions show hints of blue, possibly associated with younger stars and ongoing star formation in the disk. No strong tidal features or prominent spiral arms are apparent, leading to the interpretation that this is a relatively evolved galaxy.
