The galaxy presents a relatively smooth and featureless appearance in this image. Its morphology is broadly elliptical, appearing somewhat flattened, but not exhibiting a clear disk structure. The galaxy's light is concentrated towards the center, forming a bright, diffuse core. The color gradient transitions from a bluer hue in its outer regions to a redder hue toward its core. The overall color suggests a stellar population dominated by older, redder stars, with a potentially declining rate of star formation. There are no obvious signs of spiral arms, bars, or significant dust lanes. No major merging or tidal disturbances are apparent.
