The galaxy presents as a centrally concentrated, relatively smooth structure. It appears elliptical in shape, with a slightly elongated profile. The core is bright and concentrated, suggestive of a significant stellar population density in the central region. The galaxy exhibits a color gradient, transitioning from a generally yellowish-white core to a bluer hue in the outer regions. There is little evidence of prominent spiral arms or substantial dust lanes. The overall morphology is indicative of a relatively evolved system, with no major signs of ongoing mergers or significant disturbances, although a very mild asymmetry cannot be ruled out. The light distribution is consistent with a galaxy that may be in the process of transitioning from actively star-forming to a more quiescent state.
