The galaxy appears as a centrally concentrated, somewhat elliptical object. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light diffuses into a fainter, bluish halo. There is a subtle hint of asymmetry, with a slight extension on one side. There are faint patches of bluer light, that may indicate regions of ongoing star formation, scattered within the broader structure. The overall morphology appears relatively undisturbed, with no obvious signs of a major merger or tidal interactions. 
