The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated with a bright, yellowish core. The isophotes are elliptical, exhibiting a moderate degree of ellipticity. The overall color suggests an evolved stellar population, with relatively little evidence of ongoing star formation. There is a hint of a disk structure present, but the galaxy is likely to be elliptical or lenticular in type. No obvious signs of strong tidal interactions or recent merger events are discernible from the image. There might be some minor disturbance present, but it does not appear to be actively merging with another galaxy.
