The galaxy presents as a somewhat elliptical, disk-like structure with a moderately bright, concentrated central bulge. The light distribution appears smooth, with a gradual decrease in intensity from the core outwards towards the edges. There is no obvious spiral arm structure or significant dust lane obscuration visible in this image. The color profile suggests a dominance of older stellar populations, particularly in the bulge region, indicated by the yellowish hue. Fainter, bluer regions may be present in the outer disk, suggestive of some ongoing, albeit low, star formation. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions.
