The galaxy presents as a relatively smooth, elongated structure. It displays a bright central bulge that appears yellowish-white in color, indicative of an older stellar population. Moving outward from the center, a faint, bluish-white disk extends, suggesting the presence of younger, hotter stars. The galaxy's overall morphology leans towards a cigar shape, indicating that it is likely an elliptical galaxy. There is a small amount of possible dust that could mean it's a lenticular type, but the image is not high enough resolution to know for sure. There is no obvious evidence of strong spiral arms or any major merging events, although there might be a very slight distortion in the disk which means it might be undergoing a minor disturbance. The light profile of the galaxy appears fairly smooth, with a gradual decrease in intensity from the center outwards.
