The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. The central region displays a bright, yellowish hue, which gradually fades into a more diffuse outer halo. The shape is generally rounded, with no apparent spiral arm structures or significant irregularities. The galaxy appears relatively isolated, with no obvious signs of ongoing mergers or tidal disturbances. The lack of distinct features suggests a population dominated by older stars and a low rate of current star formation.
