The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile suggests a dominant spheroidal component, with a high degree of central condensation. There is an indication of a possible disk that extends beyond the more spheroidal core. The galaxy exhibits a slight blue hue on one side, and the rest of the galaxy is redder in color, indicating a difference in stellar populations or dust content across the galaxy. There is no apparent evidence of ongoing major merger activity or significant tidal disturbances. However, a very slight asymmetry might suggest a minor interaction in its past.
