The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. A central bulge is suggested by a concentration of yellowish light. Fainter bluish light extending from the central region towards the ends of the galaxy suggests areas of recent star formation. No distinct spiral arms or other detailed features are discernible, indicating it may be a lenticular or early-type spiral galaxy viewed at a significant angle. The overall lack of fine detail suggests that the galaxy is at considerable distance. There is no visual indication of any major mergers or tidal disturbances. The overall colour profile indicates that it has a moderate amount of star formation, with a considerable population of older, redder stars in the central bulge.
