The galaxy presents as a relatively smooth, elliptical morphology, displaying a dominant spheroidal component. The light distribution suggests a high degree of central concentration. The galaxy appears yellowish-orange in color, indicating an older stellar population with fewer young, massive stars. There is evidence of a possible minor interaction or tidal disturbance with a smaller companion object to the right of the main galaxy, but the galaxy also has high probabilities of being round and smooth. Star formation is suspected to be very low. It presents a system that is not undergoing significant merging activity. Overall, the system appears as a relatively evolved galaxy with a high mass.
