The galaxy presents as a moderately luminous, elongated structure, likely an elliptical or lenticular galaxy, viewed at an oblique angle. The central region exhibits a high degree of concentration of light, appearing smooth and featureless. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness, with a smooth transition to the outer regions. The color profile suggests an older stellar population, indicated by the yellowish-red hue. There is no apparent evidence of spiral arms or significant dust lanes, further supporting a classification toward the elliptical end of the Hubble sequence. The galaxy shows no obvious signs of any recent or ongoing major merger events. Slight asymmetry or minor disturbances are possibly present in the morphology of the galaxy. Overall, the galaxy appears as a relatively undisturbed system with a well-established structure.
