The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population dominated by evolved stars. There is little indication of spiral arm structures or significant dust lanes. The galaxy appears relatively isolated, showing no immediately obvious signs of ongoing or recent major mergers or tidal interactions. A faint blue light is observed on one side of the galaxy, possibly indicating some ongoing star formation in that region. It appears quite round, but there may be a small extension on one side. Overall, the galaxy appears to be a relatively evolved system with a dominant spheroidal component and subdued star formation activity.
