The galaxy presents as a single, moderately bright object with a slightly elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, showing a fairly even color profile across its visible extent. There is little indication of spiral arm structure or prominent dust lanes. The galaxy’s apparent color suggests a population of older stars, though a small amount of star formation cannot be ruled out. There is no clear indication of tidal features or other signs of recent or ongoing mergers, but very minor disturbances may be present. Overall, the galaxy appears to be a relatively undisturbed, mature system.
