The galaxy presents as an elongated, cigar-shaped structure. It appears to be relatively smooth, with no distinct spiral arms or prominent dust lanes visible in this observation. A central bulge region is evident, exhibiting a concentrated intensity of light. The overall color profile suggests a population dominated by older stars, indicated by the reddish-yellow hue of the bulge. The galaxy's outer regions appear more diffuse. There is no obvious indication of a major ongoing merger. The general appearance is consistent with an elliptical galaxy or a lenticular galaxy viewed at a high inclination.
