The galaxy appears as a concentrated, bright central bulge. It exhibits a yellowish-orange hue, suggestive of an older stellar population. The overall form is smooth and somewhat elliptical. There's little indication of significant spiral arm structure, and no clearly defined dust lanes are visible. A small companion galaxy appears nearby, indicating the possibility of a gravitational interaction. Overall, it appears to be a relatively large galaxy, consistent with a higher stellar mass. The galaxy is likely undergoing moderate levels of star formation. It is relatively undisturbed, with only minor indications of morphological disturbances or ongoing merger events.
