The galaxy presents a generally smooth morphology, with a slightly elongated shape, appearing somewhere between round and cigar-shaped. It exhibits a concentrated central bulge, with color gradients suggesting older stellar populations towards the center. Fainter, bluer regions extend outwards from the core, possibly indicating areas of more recent, though not particularly vigorous, star formation. No distinct spiral arms or a well-defined disk are visible, but subtle irregularities in the outer regions suggest a potential minor disturbance. Overall, the galaxy does not appear to be undergoing a major merger event.
