The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, indicating a likely concentration of older stellar populations. The surrounding halo appears somewhat more diffuse, with a subtle gradient transitioning to a bluer color at the periphery. There is little to no visible disk-like structure or spiral arm features discernable at this resolution, suggesting an elliptical or lenticular classification. It appears generally undisturbed, showing no signs of ongoing major mergers or tidal interactions, but there is potentially minor disturbance occurring. Its overall shape is moderately rounded, lacking a highly elongated or cigar-shaped appearance.
