The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, yellowish core that gradually diminishes in intensity toward the outer regions. The galaxy's overall shape is nearly circular, displaying minimal elongation. There is a subtle hint of a disk-like structure, but it is faint and largely obscured by the dominant spheroid component.

There appears to be some tidal disturbances around the galaxy, potentially indicating past or ongoing minor interactions or mergers. A slight asymmetry in the outer halo could be indicative of a disruption. No prominent spiral arms or strong star-forming regions are discernible within the galaxy. The color suggests a population of older stars. The galaxy exhibits a red shift, indicating that it is moving away from us.