The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular classification. Its shape appears somewhat elongated, but leans toward being generally roundish. There is a subtle disturbance or irregularity that may be indicative of a very minor interaction or internal process. Based on its color index and inferred star formation rates, the galaxy exhibits intermediate star formation activity with the stellar population of the galaxy likely trending towards the redder end of the spectrum, implying an older population of stars dominating its light. Its estimated size is about 7 kpc in radius. The galaxy is likely to be quite massive.
