The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The overall color appears yellowish-white, suggesting an older stellar population. There is a slight elongation, but the galaxy is generally rounded in shape. No distinct spiral arms or significant dust lanes are visible, and no obvious signs of a major ongoing merger are apparent, though there may be a slight asymmetry or minor disturbance in the outer regions. The galaxy appears to be relatively isolated, lacking any bright or obvious companion galaxies in close proximity. Star formation is likely minimal, correlating with the observed color and morphology.
