The galaxy appears as a single, concentrated object. Its color profile is generally yellow/orange, indicating an older stellar population. There is a slightly brighter yellow hue towards the center of the galaxy, suggesting a higher density of stars in the galactic nucleus. The galaxy's overall shape is largely smooth and elliptical, exhibiting a subtle deviation from perfect circularity. The shape is more rounded than cigar shaped, suggesting a relatively low degree of rotational support. There is no strong evidence of spiral arms or a prominent disk structure. There is no indication of major mergers or tidal disturbances, which would appear as distortions of the shape. Overall, the galaxy appears to be a passively evolving system with a moderately high stellar mass and low star formation rate.