The galaxy presents a generally smooth and rounded morphology, with a concentrated central bulge. The light profile suggests a relatively even distribution of stars across the galaxy, with a slight elongation visible. Color gradients are subtle, but there is a suggestion of a redder hue towards the central region, potentially indicating an older stellar population or increased dust obscuration. The outer regions appear bluer, possibly indicating the presence of younger, hotter stars. No distinct spiral arms or other prominent features are readily apparent. Overall, the galaxy appears to be an elliptical galaxy with a substantial stellar mass and relatively low current star formation activity.
