The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated bulge or core region. The overall shape appears close to circular, with minimal elongation. The color profile suggests the presence of an older stellar population, particularly concentrated in the central regions, with a yellowish to orange hue. Fainter, bluer regions exist in the outer edges. The galaxy does not appear to display significant signs of ongoing mergers or major disturbances, but some slight irregularities indicate potentially minor disturbances.  There are slight hints of disk-like features, but the galaxy is overall bulge-dominated and the disk is faint.
