This galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The bulge exhibits a slightly blueish hue in comparison to the rest of the galaxy, indicating the possibility of a population of younger, hotter stars. The outer regions of the galaxy appear less defined, fading into the background sky, but there is a slight hint of disk-like structure. No strong spiral arms are visible, nor are any obvious signs of a recent major merger event like tidal tails or prominent distortions in the overall shape. Based on the moderately bright central bulge, this galaxy may be a somewhat massive galaxy.
