The galaxy presents as an elongated structure with a relatively smooth overall appearance. The central region exhibits a bright, concentrated luminosity suggesting a high density of stars or an active galactic nucleus. The galaxy is not perfectly circular in projection; there is some degree of ellipticity. The light is not uniformly distributed across the galaxy. The outer regions appear fainter and more diffuse, indicating a lower stellar density. There appears to be some degree of disturbance or tidal feature, suggesting possible interactions with another galaxy. There is evidence of both older stellar populations (yellow/red hue) and pockets of possible younger, bluer star formation.
