This galaxy presents as a relatively compact, elliptical object. The light is dominated by a bright central core with a strong concentration of light. There appears to be a faint, diffuse halo extending outwards from the core. The halo appears to be relatively smooth, lacking any distinct spiral arms or bar structures.

The color profile exhibits some variation. The central core appears bluer, possibly indicating a younger stellar population or increased star formation. The outer regions display a more reddish hue, potentially signifying an older, redder stellar population.

There are potential signs of minor disturbances or tidal interactions present in the outer halo, though these are not strongly pronounced. The overall shape is largely regular, supporting a classification of an elliptical galaxy with some indication of possible past interaction.
