The galaxy appears as a relatively compact, elliptical-like structure. The light profile suggests a smooth distribution of stars, with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, indicating the presence of an older stellar population or possibly emission from an active galactic nucleus. A slight color gradient is observable with the outer regions displaying a faint bluish tinge, possibly indicating some ongoing star formation. The galaxy appears largely undisturbed, lacking any prominent tidal features or signs of recent mergers. There is a slight asymmetry, however the general shape is round.
