The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of luminosity, suggesting a concentration of stars. The light from the galaxy appears somewhat homogenous, showing a gradual decrease in brightness from the center to the outer edges. There is little to no evidence of distinct spiral arms or significant dust lanes. Overall the galaxy shows a somewhat round morphology, with hints of a possible very slight deviation towards a more elongated shape. It is relatively isolated, showing no indications of any ongoing major mergers or strong tidal disturbances.