The galaxy appears to be a relatively smooth, elliptical type. It exhibits a central bulge that is bright and concentrated, surrounded by a less defined, more diffuse halo. There is a hint of a disk component, though it lacks distinct spiral arms or bar structure. The overall color is bluish-white, suggesting a population of younger, hotter stars, but with a subtle reddening towards the outer regions. The galaxy's form is slightly elongated, with a moderately high degree of central concentration. There is no obvious visual evidence of a major merger or significant tidal disturbances. The galaxy does not appear perfectly round; rather it is observed to be elliptical with the shape being described as "in between", rather than completely round or cigar-shaped.
