The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright, and yellowish core, which may indicate an older stellar population. The light gradually diffuses outwards, transitioning from yellowish to a greenish hue, possibly suggestive of younger stars or a small amount of ionized gas. There are hints of a very faint disk-like structure, but overall the galaxy lacks prominent spiral arms. A slight elongation is observed, appearing more in-between round and cigar-shaped. The overall color suggests a relatively quiescent star formation rate, with the majority of stars being older. There is no visual evidence of major mergers, but there may be indications of minor disturbances.
