The galaxy presents as a somewhat diffuse, elliptical-like structure. It exhibits a concentrated central bulge which is yellowish, indicating a population of older stars. Fainter bluish light surrounds this core, suggesting the presence of a relatively low amount of younger, star-forming regions. The overall shape appears slightly disturbed, which could indicate a past or ongoing minor interaction with another galaxy. There is no clear spiral structure apparent; the distribution of light is smooth. The faintness of the outer regions implies a moderate distance and the presence of a substantial halo component. The galaxy is a relatively massive system with a moderate rate of star formation. It shows no sign of active galactic nuclei activity. The general morphology suggests that this galaxy has largely completed its major merging activity and is now in a relatively stable state.
