The galaxy appears to be a relatively compact object, with a smooth, elliptical morphology. The light distribution is dominated by a central bulge, which appears near spherical. The color indices suggest the presence of an older stellar population, potentially indicating that star formation activity is currently suppressed within this system. There are no obvious signs of spiral arms or a significant disk component. Minor irregularities in the light distribution may hint at past or ongoing interactions, however the general symmetry of the galaxy favors a non-disturbed state. The estimated size of approximately 6.6 kpc suggests this is a dwarf galaxy.
