The galaxy presents a largely smooth morphology, with a high degree of central concentration. The light profile appears elliptical, closely approaching a circular form. There is a notable lack of any distinct disk or spiral arm structures. Color gradients suggest a predominantly older stellar population, with a yellow-red hue in the central region. The outer regions exhibit a subtle fading in intensity and slightly bluer color, suggestive of possible recent, but subdued, star formation activity at a low rate. There is no evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity.
