The galaxy presents a largely smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing more elongated than circular. The color profile suggests a population of older stars, with a subtle blue hue. No distinct spiral arm structures are apparent, nor any obvious signs of ongoing major mergers or significant tidal disturbances. There might be a slight indication of a minor disturbance or interaction, but further observations are required to ascertain this accurately. The overall appearance is consistent with a relatively quiescent system.
