The galaxy presents a largely elliptical morphology, exhibiting a high degree of central concentration. There appears to be little to no disk component visible. The galaxy's light profile is smooth with no obvious spiral arm structure or dust lanes, suggesting a relatively evolved system. The core is bright and somewhat yellowish, indicating an older stellar population dominating the central region. Moving outward from the core, the galaxy exhibits a slight colour gradient, transitioning to a redder hue, which might suggest subtle metallicity or age variations within the galaxy's stellar populations. The outer regions of the galaxy fade gradually into the background, with a high degree of axial symmetry.
