The galaxy presents as a relatively smooth, elliptical-like structure with an apparent lack of significant spiral arms or a prominent disk. The light distribution is concentrated towards the center, suggesting a prominent bulge. The overall color appears to be moderately red, hinting at an older stellar population and a lower rate of ongoing star formation. There are some slight irregular features that suggest possible minor disturbances, however no major merging events are visible. The galaxy has an estimated size of about 2.6 kpc.
