This galaxy appears to be relatively compact, displaying a centrally concentrated luminosity profile. The galaxy's morphology is somewhat ambiguous, possibly exhibiting a slight degree of asymmetry. It displays a relatively smooth appearance, hinting at an elliptical or lenticular classification. A small amount of faint structure in the form of slight tidal tails may indicate past or ongoing gravitational interactions. The blue-green hue of the galaxy suggests the presence of some star formation or perhaps a contribution from an active galactic nucleus. A slight disk structure or faint spiral arm could be present, however, the low resolution makes it difficult to definitively classify this galaxy. 
