The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. The overall color appears slightly reddish-yellow, indicative of an older stellar population or a significant amount of dust obscuration. There is little evidence of distinct spiral arms or other features associated with disk galaxies. The galaxy appears to be isolated with no obvious signs of ongoing major mergers, though there is a slight asymmetry suggesting minor disturbances or past interactions. The galaxy exhibits a somewhat round shape.
