The galaxy presents as a single, largely homogenous body with a smooth appearance. It exhibits a concentrated central bulge, with a noticeable decrease in luminosity moving outwards. The galaxy appears largely spheroidal in shape with a slight elongation. Color gradients are subtle, with the core displaying a yellowish hue, suggestive of an older stellar population. This transitions towards a bluer tinge in the outer regions, potentially indicating the presence of younger stars or ongoing, but subdued, star formation. There is no visual evidence of prominent spiral arms, bars, or tidal disturbances suggesting it is likely an elliptical galaxy, and it is not currently undergoing a major merger event. Overall, it seems to be a rather quiescent system.
