The galaxy presents a predominantly smooth, elliptical morphology, displaying a slightly elongated, cigar-shaped structure. The central region exhibits a concentrated, bright core, suggestive of a significant stellar population and/or active galactic nucleus. The color gradient transitions from a yellowish core to a subtly bluer, fainter outer envelope. There is faint evidence of minor tidal disturbances or interactions, possibly indicating past or ongoing mergers, though the overall structure remains largely undisturbed. The disk component, if present, appears heavily inclined or significantly diminished. Star formation is likely present, but at a subdued rate. The estimated stellar mass is very high.
