The galaxy presents an elongated, cigar-shaped morphology, suggesting it may be an elliptical galaxy viewed at an angle. The light distribution is relatively smooth and centrally concentrated, displaying a gradual decrease in surface brightness from the core outwards. The core appears yellowish-white, potentially indicating a population of older stars. There's a subtle color gradient across the galaxy; the outer regions appear slightly redder than the core. The disk, if present, is not clearly resolved into distinct features such as spiral arms or prominent dust lanes. There's no obvious indication of recent major merger activity or significant tidal disturbances. Overall, the galaxy appears to be a relatively quiescent system.
