The galaxy appears to be an elliptical galaxy, exhibiting a largely spheroidal morphology. It has a smooth, diffused appearance with no readily discernible spiral arms or prominent disk-like structure. The central region presents a concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus, though the resolution does not permit definitive identification. A color gradient is present, shifting from a yellower hue in the core to a slightly bluer tint in the outer regions. This could indicate a variation in the age and metallicity of the stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars populating the outskirts, although the effect is subtle. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity.
