The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution indicates it is more elongated than perfectly circular, possibly taking on a cigar-like shape. The central region is the brightest, with the luminosity gradually decreasing towards the outer edges. There is a subtle color gradient across the galaxy, with the core appearing slightly redder than the outer regions. No distinct spiral arms or prominent dust lanes are visible. There are no signs of ongoing major mergers, although minor disturbances cannot be ruled out. The galaxy appears isolated, with no immediate companion galaxies exhibiting strong tidal interactions.
