The galaxy presents as a concentrated, centrally luminous object with a generally elliptical morphology. The light appears to be dominated by older stellar populations, indicated by the yellow-orange hue of its central regions. There is some evidence of extended structure or tidal features, likely resulting from gravitational interactions with a potential merging event. These regions exhibit a slightly bluer color, hinting at the presence of some younger stars. Overall, the galaxy is a complex system displaying characteristics that place it somewhere on the continuum between a smooth elliptical galaxy and one undergoing a significant merger. It is likely a fairly massive galaxy with very little new star formation.