The galaxy presents a largely smooth, elliptical morphology. A bright central bulge is apparent, transitioning into a fainter, diffuse halo. There is no clear disk structure, and spiral arms are absent. The color gradient suggests an older stellar population, with the central bulge exhibiting a more yellow/red hue compared to the bluer, albeit faint, outer regions. No distinct dust lanes or signs of active star formation regions are readily visible in the image. The overall appearance implies a relatively quiescent system with minimal ongoing merger activity or significant structural disturbances. Its shape is roughly in between a cigar and round.
