The galaxy presents as a relatively smooth, disk-like structure with a pronounced central bulge. The dominant color is a yellow-orange hue concentrated in the central region, suggesting an older stellar population. A subtle color gradient is visible from the center outwards, with the outer regions displaying a slightly bluer tint. This indicates the presence of younger stars and potentially ongoing star formation in the periphery. The disk appears somewhat elongated, transitioning between round and cigar shaped, hinting at a possible inclination relative to the observer's line of sight. There is some evidence of minor disturbances in the surrounding morphology, potentially indicating past interactions or minor mergers. Overall, the galaxy appears to be a massive galaxy that is relatively evolved, potentially transitioning from a spiral to an elliptical morphology.
