The galaxy appears to be a relatively smooth, elliptical galaxy, viewed at an oblique angle. The overall color is yellowish-white, suggestive of an older stellar population. There is a slight elongation visible, indicating a deviation from perfect circularity. No distinct spiral arms or prominent dust lanes are discernible. The galaxy exhibits a centrally concentrated luminosity profile that gradually fades toward its outer regions. There are no signs of significant ongoing mergers or major tidal disturbances in its immediate vicinity, though there are some minor artifacts that might be indicative of a slight gravitational disturbance.
