The galaxy appears to be an elliptical galaxy. It presents a generally smooth, centrally concentrated light profile with no discernible spiral arm structure or prominent disk features. The galaxy exhibits a slightly elongated, almost circular shape, with a smooth transition from a bright, reddish core to a more diffuse, bluish outer halo. There is no indication of any major mergers or significant tidal disturbances in the immediate vicinity. The red hue in the central regions suggests an older stellar population, while the bluer tones in the outer regions may indicate the presence of younger stars or residual star formation activity. The galaxy's overall appearance indicates a relatively evolved system.
