The galaxy presents a generally smooth morphology. The light profile suggests a concentrated spheroid, characteristic of an elliptical galaxy or a bulge-dominated spiral. There is a slight elongation, but overall the galaxy is fairly round. No distinct spiral arm structures or dust lanes are visible. The color appears predominantly yellow/red, indicating an older stellar population and lower current star formation rate. There is no obvious evidence of tidal disturbances or ongoing major mergers. However, there is some slight asymmetry. The galaxy appears relatively undisturbed, with the bulk of the light smoothly distributed.
