The galaxy presents as a centrally concentrated object, approximately round in shape, with a smooth overall texture. The central region exhibits a bright, dominant core, suggesting a significant concentration of stars. The light distribution appears to fall off gradually from the center. Faint, diffuse regions of light extend outwards from the central core, possibly hinting at a faint disk. There are indications of minor disturbances or irregularities in the outer regions, but they do not appear to be involved in a major merging event.
