The galaxy presents as a luminous, elliptical object with a significantly bright central bulge that fades gradually towards its outer regions. The overall color is yellowish-orange, suggestive of an older stellar population. There is little to no visible evidence of distinct spiral arms or significant dust lanes; this supports a classification toward the elliptical end of the Hubble sequence. It appears relatively smooth in texture, with a subtle elongation along one axis and a high degree of central concentration of light, indicating it is likely a high Sersic index galaxy. There are no obvious tidal features, strong distortions, or nearby companion galaxies that would indicate a recent or ongoing major merger event, though subtle disturbances cannot be ruled out.
