The galaxy presents an elliptical morphology, appearing somewhat elongated in shape. The light distribution is concentrated toward the center, exhibiting a smooth profile that suggests an older stellar population. There is some indication of a disk, possibly an older redder disk, and one side of the galaxy exhibits a smooth tidal tail, possibly indicating a minor disturbance from an ongoing or recent merger event. Overall, this galaxy displays features consistent with a relatively massive system undergoing or having recently undergone an interaction.