The galaxy appears to be a relatively smooth, centrally concentrated object. There is little discernible spiral structure or strong evidence of active star formation regions. The central bulge is prominent and bright. A faint, diffuse halo surrounds the core, suggesting a lack of significant dust lanes or obscuring material within the galaxy. The overall color is slightly red, which could indicate a relatively older stellar population and a lower rate of ongoing star formation. There are subtle features or irregularities in the galaxy's outer regions, possibly indicating a minor gravitational interaction or past merger event. The galaxy has a generally elliptical appearance, leaning towards round rather than elongated.
