The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, exhibiting a high degree of radial symmetry. The core of the galaxy displays a bright, intense luminosity, suggesting a significant stellar density. The light profile fades gradually from the core outward. There is some evidence of faint, diffuse structure in the outer regions, possibly indicating a halo or extended stellar population. The color appears primarily white, with a slight hint of blue in the outer regions. No distinct spiral arms, bars, or dust lanes are discernible, consistent with an early-type morphology. There are some subtle distortions in the outer isophotes, hinting at a possible past minor merger event. The overall impression is that of a mature, quiescent galaxy with little ongoing star formation.
