The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a near-spherical morphology, with a gradual decrease in surface brightness from the core outwards. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region. Fainter, bluer colors appear at the outer edges, which may indicate some ongoing star formation, though this is not obviously apparent. There are no readily discernible spiral arms or a distinct disk structure. The overall impression is that of a massive, evolved galaxy, likely an elliptical or lenticular type. The absence of significant tidal features suggests that it is relatively isolated and undisturbed. There is some subtle asymmetry present, but it is minimal. The galaxy lacks a very bright core, showing a more gradual and faint change in intensity towards the central region.
