The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellow-white in color, indicative of an older stellar population. The radial color profile suggests a gradual transition from a bluer inner region to a redder outer halo. There is a subtle asymmetry in the galaxy's light distribution, possibly indicative of minor tidal interactions or internal processes. No distinct spiral arms or significant dust lanes are visible. The galaxy shows an inclination between round and somewhat elongated, suggesting a viewing angle that is not precisely face-on or edge-on. There is no evidence of a major ongoing merger, though minor disturbances cannot be ruled out. The overall color suggests that star formation is likely suppressed.
