The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish-white hue, suggesting an older stellar population dominating the central area. There is a gradual decline in surface brightness moving outward from the core, with the outer regions showing a fainter, somewhat bluer tint, potentially indicating a more recent, though limited, amount of star formation. No distinct spiral arms or prominent dust lanes are discernible within the resolution of the image. Overall, the galaxy presents a relatively undisturbed structure, lacking obvious signs of ongoing major merger activity, though subtle irregularities in the outer halo cannot be entirely ruled out at this resolution.
