The galaxy presents as a singular, somewhat spherical object with a concentrated central bulge. The light distribution is relatively smooth, with a clear peak in the central region that fades into a more diffuse halo. The color is predominantly yellowish-orange, suggesting a stellar population dominated by older, redder stars, though there is a subtle hint of bluer light in the outer regions, potentially indicating some ongoing star formation. There is no apparent dust lane or spiral structure, further supporting the observation that this is a more spheroid morphology. No significant tidal tails or other disturbances are observed, suggesting the galaxy is not currently undergoing a major merger event. There might be minor interaction or disturbances, but if that is the case, they are very minor. The overall impression is that of an elliptical galaxy in a relatively quiescent state.
