The galaxy appears as a smooth, elongated structure. The central region exhibits a bright, concentrated light profile, suggesting a prominent bulge component. The outer regions appear fainter and more diffuse, extending along the major axis of the elongated shape. The color gradient suggests an older stellar population dominating the galaxy's composition, indicated by a redder hue in the central region. There's no obvious spiral arm structure or dust lanes visible. The galaxy appears undisturbed, with no indications of major ongoing mergers or tidal interactions.
