The galaxy presents as a relatively smooth, elliptical structure, with a prominent, bright central bulge. The overall color appears to be bluish, suggestive of a moderate amount of ongoing star formation. The light is concentrated toward the center, indicating a high stellar density in the nucleus. There is minimal visible evidence of spiral arm structure or a distinct disk component. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or significant tidal distortions. Faint extensions or irregularities may be present at the periphery, but it is difficult to say for certain.
