The galaxy appears as a smooth, elongated structure, resembling a cigar shape. It presents a concentrated central bulge that graduates outward into a broader, yet less defined disk. The color profile exhibits a gradient from a yellow-orange core indicative of older stellar populations to a slightly bluer halo which might imply the presence of some ongoing star formation activity. There are no signs of major disturbances or tidal features suggestive of recent major mergers, though minor asymmetry hints at a possible past interaction. The high degree of smoothness suggests that the galaxy is likely a lenticular or early-type spiral galaxy.