The galaxy presents as a primarily smooth, elliptical structure with an apparent round morphology. It exhibits a dominant central bulge, highly concentrated and bright, gradually fading toward the outer edges. There are no prominent spiral arms or significant dust lanes visible. The galaxy's color profile suggests an older stellar population, with a yellow-orange hue indicative of evolved stars. Faint disturbances or tidal features are potentially present in the halo, indicating a possible history of minor interactions, but these features are not immediately apparent. The estimated size of the galaxy is relatively large, suggesting a substantial physical scale. Overall, the galaxy appears to be a massive elliptical galaxy with little ongoing star formation.
