The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge exhibiting a yellow-white hue, suggestive of an older stellar population. The galaxy appears elongated, with a ratio of major to minor axis that suggests a classification tending towards an elliptical type. There is little evidence of spiral arm structure or significant dust lanes within the observable portion of the galaxy. The galaxy has a faint blueish color in the outer regions. No signs of major mergers or tidal disturbances are readily apparent, although minor asymmetries cannot be ruled out based on this image alone. The outer halo appears to be rather diffuse, gradually fading into the background sky. Overall, the galaxy seems to be a fairly regular and well-formed elliptical galaxy.
