The galaxy presents as a relatively smooth, elliptical structure. It is elongated in shape, appearing cigar-like rather than perfectly spherical. There is no apparent spiral structure or distinct disk. The color gradient indicates a concentration of older stellar populations toward the center, as the core exhibits a reddish hue. Fainter, bluer regions are distributed towards the outer edges, suggesting ongoing star formation in these areas, albeit at a modest rate. There is no clear evidence of major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out.
