This galaxy presents as a luminous, relatively smooth object, exhibiting a centrally concentrated morphology. The galaxy's light profile is characterized by a strong central bulge, which transitions into a more diffuse, extended halo or disk. The bulge displays a yellowish hue, indicating an older stellar population likely dominated by red giant stars. The outer regions appear bluer, possibly indicating regions of ongoing or recent star formation. Some irregularities or minor disturbances are suggested, though not strongly defined. The galaxy's shape appears to be in between a circular and elongated state. There is no clear evidence of a major merger or significant tidal disruption, although a minor disturbance could be taking place.
