The galaxy presents as a slightly elongated, centrally concentrated object. Its overall color is yellow, suggesting an older stellar population with fewer young, hot stars. There is no distinct spiral arm structure visible, implying a lack of ongoing, significant star formation in a disk. The galaxy appears relatively smooth with no obvious dust lanes or regions of intense star formation. It is not perfectly round, exhibiting a mild ellipticity. There is no obvious evidence of any major mergers or tidal disturbances that would cause asymmetrical features.
