The galaxy exhibits a generally smooth morphology, with a dominant, centrally concentrated bulge component. The light distribution suggests an elliptical or lenticular classification, displaying an overall rounded appearance with a minor elongation. There is a notable absence of prominent spiral arm structures. While appearing mostly undisturbed, subtle asymmetries within the light profile hint at potential minor interactions or recent accretion events. The object demonstrates a yellowish hue, indicative of an older stellar population and a relatively quiescent star formation rate. The galaxy possesses a considerable mass, suggesting a mature system residing in a relatively dense environment.
