The galaxy presents as a smooth, elongated structure with a concentrated central bulge. The color gradient transitions from a yellowish core to a bluer hue in the outer regions. This suggests the presence of older stellar populations in the center and relatively younger stars in the outer disk or halo. There are no readily apparent spiral arm structures or significant dust lanes visible in the image. The overall form leans toward being cigar-shaped, appearing significantly longer than it is wide. There appears to be little to no signs of ongoing major mergers, or any signs of significant tidal distortions or disruptions in its morphology. The light distribution of the galaxy seems fairly symmetrical around its major axis.
