The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The central region exhibits a brighter, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the galaxy's color transitions towards a bluer tinge within the outer regions. There is no apparent spiral structure. The outer regions show a gradual decline in luminosity, blending smoothly with the surrounding background. There are no obvious signs of significant tidal disturbances or ongoing major merging activity. The galaxy appears well-defined, indicating a mature and relatively undisturbed system.
