This galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright and yellowish, suggesting a population of older stars. The overall shape is fairly round, with only a slight deviation toward a more elongated form. There is little evidence of spiral arms or significant dust lanes. A faint, diffuse halo extends outward from the central region, gradually fading into the background. There is no apparent indication of any major merging events or significant tidal disturbances in the immediate vicinity, though a possible minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively quiescent system with minimal ongoing star formation.
