The galaxy presents as a generally elliptical structure, exhibiting a dominant spheroidal component. The central bulge is prominent and appears to be composed of older stellar populations, suggested by its yellowish-white color. Proceeding outwards from the center, a subtle disk is visible, displaying a slightly bluer hue, possibly indicative of more recent star formation activity. There are no prominent spiral arms visible, indicating the system is not a grand-design spiral. The galaxy's shape is not perfectly circular but elongated, with a major axis noticeably greater than the minor axis. Overall, this galaxy exhibits a smooth appearance, hinting at the possibility of it being an early-type spiral galaxy. There are also hints of minor disturbances, possibly indicative of a previous merger event. The outer regions of the galaxy appear fainter, with a gradual decrease in surface brightness towards the edge. The presence of blue light indicates that there is still some low level of ongoing star formation within the galaxy.
