The galaxy presents a generally smooth and concentrated morphology. Its overall form appears to be elliptical, exhibiting a high degree of radial symmetry. The light distribution is centrally concentrated with a gradual decrease in surface brightness moving outward from the core. The core region displays a bright, yellowish hue, suggesting a significant population of older stars. Moving outward, the color transitions subtly to a more reddish tone, though this is somewhat subtle. There is no indication of prominent spiral arms, bar structures, or active star formation regions, at least within the limits of the image resolution. The overall appearance suggests a relatively evolved system with a dominant population of older stars and a quiescent star formation rate. The presence of minor disturbances cannot be entirely ruled out based on the image, but the overall structure appears to be relatively undisturbed.
