This galaxy appears to be a lenticular type, presenting a flattened, disk-like morphology. Its overall color profile is indicative of an older stellar population, primarily exhibiting redder hues, which suggests a reduced rate of ongoing star formation. The galaxy's light is relatively smooth and centrally concentrated, showing a distinct bulge, and a disk that fades gradually into the surrounding sky, exhibiting no well-defined spiral arm structures. There may be a slight asymmetry, suggesting a recent or ongoing minor interaction, though no clear tidal features are apparent.
