The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, featureless morphology. Its overall color profile is slightly redder, which could indicate an older stellar population and potentially a lower rate of on-going star formation. The galaxy's light is concentrated toward the center, suggesting a dense central bulge, and fades gradually outward. It appears to be relatively undisturbed, displaying no signs of major mergers or strong tidal interactions, although there might be some minor asymmetry suggesting previous minor disturbances. It is somewhat elongated in shape, being neither perfectly spherical nor highly flattened.
