This galaxy presents as a relatively compact, elliptical system. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density, possibly indicative of an older stellar population. The radial color profile shows a distinct trend, transitioning from a yellowish core to a slightly bluer halo. This may point to ongoing, though limited, star formation in the outer regions, or a variation in stellar metallicity. There's no clear evidence of spiral arms or a distinct disk structure. The overall morphology suggests a classification toward the early-type end of the Hubble sequence. The galaxy appears relatively undisturbed with no obvious signs of recent or ongoing major mergers.
