The galaxy presents as a centrally concentrated, elliptical morphology. The light distribution appears relatively smooth, with no discernible spiral arms or distinct dust lanes visible in the image. The galaxy exhibits a moderate ellipticity, appearing somewhat cigar-shaped, and there is no evidence of any major mergers or significant tidal disturbances. The overall color is somewhat red, indicating an older stellar population and lower levels of star formation. The galaxy has a measurable angular size and is likely a considerable distance from our own.
