The galaxy presents a primarily smooth morphology, suggesting an elliptical classification. The light profile appears concentrated, with a bright central bulge that diminishes gradually towards the outer regions. The overall shape deviates slightly from perfectly circular, appearing somewhat elongated, hinting at a possible classification of type E4-E5 on the Hubble sequence. There is evidence of a minor disturbance or interaction, potentially from a small, nearby companion which seems to be causing some tidal distortions. Color indices suggest the presence of an older stellar population, typical of elliptical galaxies, although some blue light emissions are present around the main body of the galaxy. Overall, this galaxy exhibits characteristics of an intermediate to massive elliptical galaxy that has possibly undergone a minor merger event.
