The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, somewhat diffuse glow, indicating a high stellar density and potential presence of an active galactic nucleus. The galaxy’s overall shape appears elliptical, though with a slight elongation. There is a color gradient visible, transitioning from redder hues in the core to somewhat bluer tones in the outer regions, which might imply differing stellar populations. The outer edges of the galaxy fade gradually into the background, lacking any sharp or well-defined spiral arm structures. There is no evidence of major ongoing mergers or significant tidal disturbances in the immediate vicinity of the galaxy. Faint, diffuse light extends outwards from the main galactic body, possibly indicating a halo of older stars.
