The galaxy presents as a slightly elongated, lenticular or early-type spiral galaxy. The color profile indicates a dominant population of older stars, evidenced by the yellowish-orange hue, primarily in the central bulge. No distinct spiral arm structures are discernible, suggesting a smooth, relatively featureless disk or spheroid. The central bulge appears bright and concentrated. There is little to no evidence of active star formation regions or dust lanes visible within the galaxy. The galaxy appears relatively isolated, with no immediately apparent signs of tidal interactions or ongoing mergers with other galaxies. Overall, the morphology suggests a galaxy that has largely exhausted its gas supply for star formation.
