The galaxy exhibits a generally smooth morphology. It appears elliptical in shape, with a centrally concentrated, bright core transitioning to a more diffuse halo. There is an indication of some spiral structure or disk feature. The color gradient suggests an older stellar population in the central region, indicated by the yellow-orange hue, possibly indicative of a higher concentration of evolved stars and a lower rate of star formation. Fainter blue tones present in some areas point towards the possible existence of younger star populations in the extended disk. There's no clear sign of significant tidal distortions or ongoing major mergers, although minor disturbances cannot be ruled out. The galaxy displays an apparent roundness, not appearing overly elongated or cigar-shaped.
