The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. There is a slight elongation, but overall it appears quite round. The color is predominantly yellowish, suggesting an older stellar population. Subtle hints of disturbances can be seen in the outer regions, which indicate possible minor interactions. There appears to be a secondary object nearby that could be related to the possible disturbances. Overall, it seems to be a relatively passive galaxy with indications of a possible past merger event.
