The galaxy appears as a centrally concentrated object, exhibiting a largely spheroidal morphology. There is no readily apparent disk structure, nor are there any spiral arm features visible. The galaxy exhibits a smooth profile, with a slight elongation that deviates from a perfectly circular form, but is not significantly cigar-shaped. The light distribution suggests a centrally concentrated bulge component. There are no clear signs of any major tidal disturbances, significant asymmetries, or indications of recent or ongoing major merger activity. Faint blue light is visible on the outskirts of the galaxy, which suggests that there is some amount of star formation occurring. 
