The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with a Sersic index greater than 3, suggesting a de Vaucouleurs profile. It appears moderately flattened. The galaxy's color profile indicates a redder core, transitioning to slightly bluer hues in the outer regions. This could be due to an older stellar population concentrated in the center, with younger, bluer stars contributing to the outskirts. There is no discernible evidence of spiral arms, bar structures, or ongoing major mergers. There is some indication of minor disturbance of the galaxy. The galaxy appears to be of considerable mass, and shows signs of moderate star formation.
