The galaxy appears to be a relatively smooth, elliptical system. Its morphology is dominated by a centrally concentrated bulge that fades gradually into a more diffuse halo. There is a slight ellipticity to the overall shape, indicating it is not perfectly spherical. The core is quite bright, suggesting a high density of stars or potentially an active galactic nucleus. The color profile exhibits a gradient, with a yellower hue in the central regions that transitions towards a slightly bluer tint in the outer halo, indicating a potential difference in stellar populations or dust content between these regions. There is no clear evidence of spiral arm structures or significant dust lanes. The general appearance suggests a passively evolving system.
