The galaxy presents a generally smooth morphology, suggestive of an elliptical galaxy type. It exhibits a centrally concentrated luminosity profile, with a bright, well-defined core. The overall shape approximates a circular form, showing little deviation from rotational symmetry. The colour distribution is centrally biased toward redder wavelengths, transitioning to slightly bluer hues in the outer regions, possibly indicative of an older stellar population in the core with younger stars further away from the center. There is no obvious evidence of spiral arm structure or significant dust lanes. There are no visible signs of tidal disturbances or interactions with other galaxies, indicating a relatively isolated system.
