This galaxy appears to be an elliptical galaxy, classified by its generally smooth light distribution. The galaxy exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outward. The core is bright, suggesting a high density of stars. It is relatively featureless, showing no prominent spiral arms or dust lanes. Its elongated shape indicates it is not perfectly spherical, but more of a flattened spheroid. There is a slight possibility of a minor disturbance event in the galaxy's past, but is currently stable. Overall, this galaxy is characteristic of an evolved system with a significant population of older stars and a relatively low rate of star formation.
