The galaxy presents as a concentrated, centrally brightened object with a smooth, largely featureless morphology. The light distribution appears primarily elliptical, with a moderate degree of roundness. There are no obvious spiral arm structures or prominent dust lanes visible. The color profile indicates a yellowish central region, potentially indicative of an older stellar population. The galaxy displays a relatively undisturbed appearance, with no readily apparent signs of a major ongoing merger. However, there is some slight asymmetry that indicates there may be minor disturbances present. These disturbances are not large enough to be considered a major merger event.
