The galaxy presents an overall elliptical morphology with a smooth appearance. The central bulge is prominent and exhibits a yellowish-white hue, suggestive of an older stellar population. A faint, flattened disk structure surrounds the bulge. The disk displays a bluer color than the central bulge, potentially indicating the presence of younger, hotter stars and ongoing star formation. Some asymmetries are visible in the outer regions of the disk, hinting at possible minor gravitational interactions or disturbances. There is no strong evidence of spiral arms or a well-defined bar structure. The galaxy appears relatively isolated within its immediate environment.
