The galaxy presents a generally smooth and elliptical morphology. It appears relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal distortions in the immediate vicinity. The galaxy's light distribution is centrally concentrated, fading gradually towards the outer edges, suggesting a relatively old stellar population dominating its overall luminosity. The slight elongation indicates a moderate degree of flattening, but it doesn't present a well-defined disk-like structure. The galaxy has an intermediate color profile, a light golden color, indicating a mix of stellar populations without strong signs of very recent, intense star formation.
