The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. The galaxy's light profile is consistent with an elliptical galaxy or a spiral galaxy viewed face-on without prominent spiral arms. Its shape is roughly in between rounded and oblong, with a slight preference towards a more elongated form. There is no strong evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity; however, some minor asymmetries cannot be ruled out. The galaxy has a moderate amount of ongoing star formation. The color index indicates that the galaxy's stellar population includes both younger, bluer stars and older, redder stars.
