The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile with no discernible spiral arm structure or prominent dust lanes. Its shape is largely spheroidal, closely approaching circular symmetry. There is a strong central bulge which then fades out into a much larger but dimmer, rounded shape. The galaxy exhibits a color gradient, with the central region appearing more yellow, suggesting an older stellar population and decreased active star formation within the core. The outer regions have a slightly bluer tint, indicative of relatively younger stars in the surrounding regions of the galaxy. There is no indication of any merging activity or major disturbances in the galaxy's overall structure.
