The galaxy presents a smooth, elongated morphology, suggestive of an elliptical galaxy viewed from a slightly oblique angle. Its color profile indicates a population of older stars, with a dominant reddish-orange hue concentrated towards the central bulge. Fainter bluish tinges are observed along the outer edges of the galaxy, potentially indicating regions of more recent, albeit subdued, star formation. There is no evidence of prominent spiral arms or significant dust lanes. No strong tidal features or distortions are observed, suggesting the galaxy has likely not undergone a recent major merger event. The general appearance of the galaxy indicates a system which is primarily spheroid, and is in a relatively quiescent state.
