The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge with a yellowish hue, suggesting a population of older stars. The outer regions exhibit a gradual decline in surface brightness, with a subtle shift towards redder colors. There is a slight elongation visible, indicating it is not perfectly spherical but rather somewhat cigar-shaped. No prominent spiral arm structures or significant dust lanes are discernible within the resolution of the image. The overall appearance suggests an evolved system with relatively low ongoing star formation activity. There are no obvious signs of major interactions or mergers, although a very subtle asymmetry might be present at the edges.
