The galaxy presents a largely smooth, elliptical morphology. It exhibits a central concentration of light that appears to be a relatively old stellar population, inferred from its reddish-yellow hue. The galaxy shows a subtle elongation, somewhere between round and cigar-shaped, but not indicative of a strong bar structure or a highly flattened disk. There are suggestions of minor disturbances or tidal features, though they are not overwhelmingly prominent, perhaps reflecting some past interaction. The overall structure indicates that the galaxy is either an elliptical galaxy or a lenticular galaxy with a substantial bulge. The colors suggest ongoing, but moderate, star formation activity.
