The galaxy presents a largely smooth, elliptical morphology. It exhibits a distinct cigar-shaped appearance. The central region displays a bright, concentrated core, suggesting a high density of stars. The color gradient transitions from a predominantly yellow-orange hue in the core to slightly redder tones in the outer regions, potentially indicating older stellar populations dominating the periphery. Some minor disturbances or tidal features may be present on the edges of the galaxy but they are rather obscured. Overall, the galaxy appears relatively isolated, showing no signs of ongoing major mergers, but some evidence of minor interactions cannot be ruled out.
