The galaxy presents a largely smooth and rounded morphology, exhibiting a concentrated central bulge. The light distribution indicates a relatively featureless structure, with no readily apparent spiral arms or significant dust lanes. There is a slight elongation to the galaxy's shape, although it maintains an overall elliptical appearance. The core exhibits a yellowish-white hue, possibly indicative of an older stellar population, while the outer regions appear slightly redder. There is no obvious evidence of recent major merger activity, though minor disturbances may be present. The galaxy shows a low rate of star formation. The galaxy appears relatively isolated, with no obvious tidal features or interacting companions.