The galaxy presents as a roughly elliptical or lenticular object with a notable central bulge. The light distribution appears relatively smooth, with a high degree of central concentration. The core region exhibits a yellowish hue, possibly indicative of an older stellar population or dust obscuration. The outer regions are fainter and have a slightly bluer tint, suggesting the presence of some younger stars, although star formation activity seems low overall. The galaxy's shape is moderately elongated, not perfectly spherical, indicating it may have some degree of rotational support. There is no obvious evidence of spiral arms or a well-defined disk structure. Likewise, there are no signs of tidal disturbances, major mergers, or strong gravitational interactions with nearby galaxies that would produce distortions.
