The galaxy presents a generally smooth, elliptical morphology. The primary light distribution is concentrated towards the center, exhibiting a yellowish-white hue suggestive of an older stellar population. It demonstrates an elongated, cigar-shaped structure, lacking distinct spiral arms or prominent features typically associated with disk galaxies. There is a slight suggestion of a bluer halo surrounding the central bulge. No major disturbances or signs of ongoing merger events are apparent in the image.
