The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. The light distribution is centrally concentrated, diminishing gradually towards the outer edges. There appears to be a slight color gradient within the galaxy, shifting from a yellowish-white hue in the core region to a bluer tint in the surrounding areas. There is a lack of well-defined spiral arm structures or prominent dust lanes. There is no strong evidence of active galactic nuclei activity, but a low level of star formation is likely occurring within the galaxy. Minor tidal disturbances may be present but are not easily discerned. The galaxy does not appear to be undergoing any major merger activity. Overall, it seems to be a relatively relaxed and evolved system.
