This galaxy presents as a centrally concentrated object, displaying a generally smooth morphology. The light profile indicates a bulge-dominated system with a gradual decrease in luminosity outward from the core. There is a subtle color gradient visible, with the central region appearing slightly bluer compared to the outer regions, which exhibit a redder hue. This may suggest some ongoing, albeit subdued, star formation activity concentrated towards the nucleus, while the outer regions may be populated by an older stellar population. There are hints of very subtle asymmetries or minor disturbances, but overall the galaxy appears relatively undisturbed. The galaxy's overall shape can be described as moderately rounded, without a distinct disk-like structure. There is no evidence of any major merging events or significant tidal interactions occurring. 
