The galaxy appears to be a relatively smooth, elliptical galaxy, approximately 5.5 kiloparsecs in effective radius. It exhibits a generally round morphology, with a slight elongation that leans towards a cigar shape. The galaxy's light profile is dominated by older stellar populations, indicated by its yellowish hue. There is no discernible evidence of a disk structure or spiral arms. The galaxy is generally undisturbed, with no major mergers or significant tidal features. The overall structure suggests a system where star formation is suppressed.
