The galaxy presents as a relatively smooth, centralized light distribution with a subtle ellipticity. It is a roughly rounded shape. The color appears to be trending towards the redder end of the spectrum, which may be due to high levels of dust obscuring the view or an older stellar population dominating the galaxy. There are some minor irregular features or asymmetries, possibly indicating a past or ongoing interaction with another galaxy. A significant portion of the light emanates from the central region. The estimated physical size indicates this is a moderate sized galaxy. The relatively low estimated star formation rate seems consistent with the red color and smooth morphology, suggesting a more evolved system where star formation is less active. The galaxy could be undergoing a minor merging event.
