The galaxy presents an elliptical morphology, though with subtle features suggesting the presence of a disk component viewed at a slight inclination. The central bulge region exhibits a bright, concentrated luminosity, appearing yellow-white in color, indicative of an older stellar population. Moving outwards, the disk shows a gradual decrease in brightness, with a bluer hue suggesting the presence of younger, hotter stars and ongoing star formation. The disk appears relatively smooth, with no distinct spiral arm structures immediately apparent, although some subtle irregularities suggest minor disturbances, possibly due to past interactions. Overall, this galaxy is a relatively massive system undergoing some star formation.
