The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution exhibits a centrally concentrated brightness, with the core region appearing significantly more luminous than the outer edges. There is no prominent disc structure, arm features, or signs of strong dust lanes visible. A subtle color gradient can be observed, with the core exhibiting a yellower or redder hue compared to the outer regions, which tend towards bluer wavelengths. The galaxy appears largely undisturbed, displaying a regular morphology with only minor indications of tidal interactions or recent mergers. There is a possibility of an early stage interaction with another galaxy, however further data would be required to verify this.
