The galaxy appears to be a relatively smooth, centrally concentrated object. It presents with a near-elliptical morphology. There may be a subtle disk-like feature but it is not well defined. The galaxy exhibits a prominent bulge, indicated by the central brightness concentration. The light profile appears smooth, with a gradual decrease in intensity from the core outwards. There does not appear to be any significant dust lanes or prominent spiral arm structure. The overall color of the galaxy appears relatively uniform, suggesting a lack of significant ongoing star formation. There is no visual evidence of a recent major merger or tidal disruption. Subtle disturbances in its structure may indicate interactions with smaller galaxies.
