The galaxy presents a generally smooth morphology, exhibiting a bright, concentrated core. The light distribution appears relatively uniform, with a slight elongation or cigar shape, though dominated by a round appearance. There is a subtle color gradient noticeable, transitioning from a yellow-orange hue in the central region to a redder color in the outer halo, indicating a shift in stellar population or dust content. No distinct spiral arms or prominent features are visible. The galaxy appears isolated, with no obvious signs of tidal interactions or ongoing mergers.
