The galaxy presents as an elliptical morphology, appearing generally smooth with a concentrated central bulge. The luminosity profile suggests a relatively even distribution of stellar populations, with a gradual decrease in brightness from the core to the outer regions. The core exhibits a yellowish hue, possibly indicating an older stellar population. The lack of prominent spiral arms or significant dust lanes suggests a classification toward early-type galaxies. There is a slight indication of minor disturbance within the galaxy with an asymmetry in the outer halo, possibly due to an ongoing or recent minor merger event. The overall color profile indicates moderate star formation within the last few hundred million years.
