This galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated with a bright, seemingly spheroidal core that gradually fades towards the outer regions. The galaxy exhibits a slight elongation, suggesting a shape deviating from a perfect sphere. There is some indication of a faint, extended disk or arm structure, visible as a subtle asymmetry in the outer regions; a very slight disruption. The colour gradient appears consistent with an older stellar population. There is no evidence of active star formation regions, such as bright blue knots or dust lanes. The galaxy presents a moderate redshift, placing it at a substantial cosmological distance.
