The galaxy presents as a spiral type, viewed at an angle oblique to face-on. It exhibits a central bulge that appears moderately sized, with a significant presence. Faint spiral arm structures are suggested, extending outwards from the central region. The galaxy displays a subtle bar feature crossing its center. The disk appears relatively smooth. The color profile indicates a dominant redder hue, likely associated with an older stellar population. No signs of major mergers are apparent, but some subtle disturbances seem to be present.
