The galaxy appears to be a relatively smooth, elliptical-like structure. The light distribution suggests a centrally concentrated morphology, with a gradual decrease in brightness outwards. The galaxy exhibits a moderate red color, hinting at an older stellar population. There may be some faint disk structure around the central bulge. No prominent spiral arms or significant dust lanes are discernible. There is a slight elongation of the galaxy's shape, however it is primarily round. There is a hint of a minor disturbance within the galaxy, but nothing substantial enough to suggest it is currently merging with another galaxy.
