The galaxy presents as a small, relatively smooth object. Its morphology appears to be generally elliptical, though with a slightly elongated, cigar-shaped profile. The light distribution within the galaxy is fairly uniform, with a gradual decrease in intensity from the center outwards. There is no evidence of spiral arms or a prominent disk structure. The galaxy exhibits a yellowish-white hue, suggesting a stellar population dominated by older, less massive stars. There are no indications of ongoing major mergers or tidal disturbances affecting the overall structure of the galaxy, although a minor perturbation cannot be ruled out. Based on the light observed, star formation appears to be low.
