The galaxy appears as a singular, diffuse luminous object. Its morphology is predominantly smooth and elliptical, exhibiting a high degree of circularity. There is little to no visual indication of spiral arms or a bar structure. The central region of the galaxy shows a slight concentration of light, indicative of a possible galactic nucleus, though it is not particularly pronounced. No prominent dust lanes or active star-forming regions are readily apparent in this image, contributing to its overall smooth texture. There is no indication of any merger activity or tidal disturbances. The observed color of the galaxy is relatively red, suggesting a population dominated by older stars with suppressed star formation.
