This galaxy exhibits an elliptical morphology, appearing largely smooth and rounded with a concentrated central bulge. There is very little discernible structure such as spiral arms or a prominent disk. The galaxy's color profile suggests an older stellar population, indicated by the redder hue and the lack of bright blue star-forming regions. Based on the apparent lack of disturbances, this galaxy appears to be relatively undisturbed, with no signs of recent or ongoing major mergers. It is likely a massive galaxy with relatively low star formation.
