The galaxy presents a morphology dominated by a smooth, elliptical form. It exhibits a centrally concentrated light profile, indicative of a significant bulge component. The overall color appears to be redder, suggesting a population of older stars and a relatively low rate of ongoing star formation. A slight elongation is visible, but the overall shape is largely rounded. There is no clear evidence of a prominent disk structure, spiral arms, or any major merger events. Minor disturbances might be present, but they are not strongly apparent in this image. The galaxy's color suggests that any recent star formation is limited in extent.
