The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated light profile, with a bright, yellowish core that gradually fades outward. The overall color suggests an older stellar population, with a diminished presence of young, blue stars. Hints of a faint disk structure might be present, but the dominant characteristic is its spheroidal nature. There is no obvious evidence of on-going major mergers or strong tidal disturbances in this image, but potentially some minor disturbances are present. The galaxy appears fairly isolated, with no obvious signs of interactions with nearby galaxies. The light distribution is somewhat elongated, suggesting the galaxy is not perfectly spherical, but rather has a slightly cigar-shaped appearance.
