The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests a population dominated by older stars, inferred from the reddish-yellow hue. There is no apparent structure suggestive of spiral arms or a prominent disk. The shape appears mostly round, with no significant elongation or distortion visible. No signs of major merging events or significant tidal disturbances are observed, and the morphology indicates that the light is not dominated by a recent or ongoing merger.
