The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge and a surrounding, less dense halo. The central region exhibits a yellowish hue, potentially indicating an older stellar population and reduced active star formation. The outer halo appears fainter with a slightly bluer tint suggesting younger stars and some ongoing star formation may be present in the outer regions. The overall morphology suggests a fairly evolved system with little sign of significant spiral structure or ongoing merger activity, though a subtle asymmetry may indicate a past interaction. The galaxy appears to be relatively isolated, with no obvious companion galaxies or tidal features nearby.
