The galaxy presents as a fairly smooth, elliptical or lenticular type object. A central bulge dominates the galaxy's structure, exhibiting a yellowish-white hue, likely indicative of an older stellar population. The light distribution becomes increasingly diffuse moving outward from the bulge, fading into a faint, extended halo. There is no apparent spiral structure or significant dust lanes visible within the image. The galaxy's overall shape appears close to round, with a slight elongation. There is no strong visual evidence of ongoing major mergers or significant tidal disturbances.
