The galaxy appears as a moderately bright, elliptical-like object, with a smooth, diffuse appearance. The central region exhibits a concentrated light distribution, potentially indicative of a substantial galactic nucleus or bulge. The galaxy displays a color gradient, with a more yellowish-orange core shifting towards bluer hues in the outer regions. This could suggest older stellar populations dominating the core, with younger, bluer stars in the galactic outskirts. A subtle, elongated morphology is observed, possibly indicative of a prolate spheroid shape. There appears to be a minor irregularity or a small, faint, feature situated on one side of the galaxy. Given the smoothness of the galaxy, this might indicate either an early stage merger with a small galaxy or a tidal disturbance caused by interaction with another object. The overall structure indicates a relatively evolved system, likely with suppressed recent star formation.
