The galaxy appears to be an elliptical type, with a smooth, centrally concentrated luminosity profile. There is little evidence of spiral arms or a disk structure. The galaxy exhibits a slightly elongated, cigar-shaped morphology, indicating a possible deviation from a perfect spheroid. The dominant color is a reddish-yellow hue, which suggests an older stellar population with fewer young, blue stars. There is no obvious evidence of a major merger or significant tidal disturbance, although a faint, subtle asymmetry might hint at a minor interaction in its past. The galaxy's light is fairly uniformly distributed across its body.
