This galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, which dominates the overall light profile. The galactic disk, if present, is not readily discernible in this image. The color appears primarily blue, hinting at a population of younger, hotter stars. The galaxy exhibits a relatively high degree of rotational symmetry. There is no clear evidence of tidal tails, shells, or other signs of recent major mergers. The isophotes appear relatively undisturbed, suggesting a relaxed dynamical state. There may be some minor disturbances to the main light body but nothing significant. The galaxy's profile is more round than cigar-shaped.