The galaxy presents as a single, concentrated object with a generally smooth morphology. The central region exhibits a bright, yellowish-white hue, possibly indicative of an older stellar population. The overall shape appears slightly elliptical rather than perfectly spherical. There is no clear evidence of spiral arms or a distinct disk structure within the observed area. Some minor asymmetry is visible, and it appears to have had at least a minor disturbance or possible signs of past merger activity.
