The galaxy presents as a somewhat smooth, elliptical morphology with a notable central bulge. It exhibits a relatively compact structure with a bright core, indicating a concentration of older stellar populations. There may be some evidence of a faint disk-like structure. The galaxy's color index suggests the presence of a substantial population of evolved stars, resulting in a reddish hue. No pronounced spiral arms or dust lanes are visible. There appears to be only minimal star formation occurring within the galaxy. Its structure is largely undisturbed, suggesting it has not undergone any recent major mergers. Overall, this is a typical elliptical galaxy in a relatively quiescent state.
