The galaxy appears as a single, relatively smooth object with a slightly elliptical morphology. There is a concentration of bluer light in the central region, possibly indicating younger stellar populations or ongoing star formation. The outer regions exhibit a redder hue, which could suggest older stellar populations or dust obscuration.

No distinct spiral arms or bar structures are clearly visible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal features, although there might be a very slight asymmetry hinting at a possible minor interaction or internal disturbance. The overall color profile suggests that this galaxy might be an early-type spiral galaxy or a lenticular galaxy, transitioning from a more actively star-forming phase to a more quiescent state.
