The galaxy presents as an elliptical or lenticular type, appearing elongated with a cigar-like shape. The central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Proceeding outwards from the center, there is a gradual decrease in surface brightness, with colors transitioning to bluish-white. This may indicate the presence of younger, hotter stars in the outer regions, though this is less pronounced. The overall structure seems relatively smooth, lacking distinct spiral arms or prominent dust lanes, though there are some faint, irregular features. These faint features are mostly concentrated in the lower half of the galaxy. The galaxy is notably compact, and the rate of star formation seems to be relatively low.
