The galaxy presents a smooth, centrally concentrated morphology. Its shape is neither perfectly round nor highly elongated, appearing somewhere in between. No distinct spiral arms or bar structures are discernible in the available image. There is no apparent major merger event, though there are minor irregularities visible in the outer regions suggesting subtle disturbances or interactions. The galaxy exhibits a relatively low rate of star formation. The overall color profile indicates a galaxy that is likely dominated by an older stellar population. The size is moderate, typical of galaxies in the intermediate mass range. 
