The galaxy appears to be an elliptical type, with a generally smooth and centrally concentrated luminosity profile. The central region displays a yellowish-orange hue, suggestive of an older stellar population. The galaxy exhibits an overall rounded shape, but also shows a slight elongation. The outer regions exhibit a faint, diffuse halo with subtle bluish tones, possibly indicating regions of younger stars or recent star formation. No distinct spiral arm structures or prominent dust lanes are visible. There may be very minor disturbances in the halo, however, the galaxy appears relatively undisturbed overall. The galaxy is of an intermediate mass, and has a medium to high star formation rate for its type.
