The galaxy appears to be a relatively smooth, centrally concentrated object with a slight elongation. The core exhibits a yellow-orange hue, suggesting a population of older stars. The outer regions of the galaxy display a fainter, bluer tint, potentially indicating the presence of some younger stellar populations. There is no obvious spiral structure or pronounced disk-like morphology visible. Subtle distortions or faint tidal features might be present in the extended halo, hinting at past gravitational interactions. No active galactic nucleus is readily apparent.
