The galaxy presents a primarily smooth morphology, with no distinct spiral arms or bar structure visible. It exhibits a roughly elliptical shape, appearing neither perfectly round nor significantly elongated. The light distribution is concentrated towards the center, suggesting a prominent bulge. A gradual decrease in luminosity is observed from the core outwards, indicating a diffuse halo or envelope. The overall color appears yellowish-white, potentially indicative of an older stellar population with ongoing, albeit subdued, star formation. There is no apparent evidence of major mergers or tidal disturbances in the galaxy's morphology.
