The galaxy presents as a relatively smooth, elliptical structure. Its morphology is primarily spheroidal, with a slight elongation resembling a cigar shape, but generally appearing rounded. There's a clear concentration of light towards the galactic center, suggesting a prominent bulge. Color gradients indicate a possible difference in stellar populations or dust content between the core and the outer regions, with the core appearing more yellowish. There are no obvious signs of ongoing major mergers or tidal disturbances, although subtle irregularities or minor disturbances cannot be entirely ruled out at this resolution. No prominent disk-like structures or spiral arms are observed.
