The galaxy presents as a relatively compact, luminous structure. Its morphology appears predominantly smooth, with a subtle central concentration of light. There is a slight elongation, suggesting it might be tending towards a mild disk-like or elliptical shape rather than being perfectly spherical. No distinct spiral arms or prominent features are immediately apparent, however, there could be signs of minor disturbance within the galaxy, possibly due to ongoing interactions with less prominent companions or an earlier merger event. The overall color is consistent with a evolved stellar population, although the brightness does indicate recent star formation.
