The galaxy presents as a centrally concentrated object with a moderately elliptical morphology. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. The central region exhibits a brighter, more concentrated core, indicative of a possible bulge or nucleus. Moving outwards from the core, the galaxy gradually fades into a more diffuse halo. While largely smooth in appearance, there are subtle variations in color and brightness in the outer regions, hinting at underlying substructure. Overall, the galaxy appears to be in a relatively quiescent state, with no obvious signs of a major merger or active star formation regions.
