The galaxy appears to be a relatively smooth, elliptical galaxy. Its central bulge is a dominant feature, exhibiting a concentrated, bright yellowish hue, suggesting a population of older stars. Moving outward from the core, the galaxy's light gradually diffuses into a less distinct halo. Faint blue tinges are visible in the outer regions, suggestive of some younger stellar populations, although not indicative of significant ongoing star formation. There is no clear evidence of spiral arm structure or a prominent disk. The overall shape appears somewhat elongated. The galaxy appears relatively undisturbed, lacking significant tidal features or signs of a major merger event.
