This galaxy presents an elliptical morphology, appearing elongated with a smooth, diffuse light distribution. A bright central bulge dominates the luminosity profile, exhibiting a yellowish hue. Moving outward from the core, the light gradually fades into a bluer disk. The galaxy does not appear to have strong spiral arm structures or significant dust lanes. There is a slight asymmetry, possibly indicating a minor gravitational disturbance or recent interaction with a smaller galaxy, though no clear signs of an active merger are immediately visible. The overall color suggests a mix of stellar populations, with older stars concentrated in the bulge and a younger population present within the disk.
