The galaxy presents a generally smooth, elliptical morphology. Its overall color is yellowish-orange, suggesting a population of older stars. There is no clear evidence of spiral arm structure, active star formation regions, or dust lanes. The light distribution appears relatively uniform, with no pronounced central bulge or disk component. The galaxy's shape deviates slightly from perfectly circular, exhibiting a subtle elongation. There is no evidence of a major ongoing merger or significant tidal disruption. The galaxy appears relatively isolated and undisturbed.
