The galaxy presents a smooth, elliptical morphology. The light distribution suggests a centrally concentrated structure with a gradual falloff in surface brightness towards the edges. It exhibits an elongated shape, more akin to a cigar than a perfect sphere. There are no obvious signs of distinct spiral arms or a prominent disk. The central region is notably brighter and appears yellower, possibly indicating a higher concentration of older stellar populations. There are no indications of major mergers or tidal disturbances in this image, however a slight irregularity to the bottom indicates possible minor disturbances. Based on the light output it is estimated to be quite massive, with moderate star formation.
