The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. There's a subtle elongation, suggesting it may not be perfectly spherical, exhibiting a cigar-like shape, but still close to round. The color gradient indicates an older stellar population; it transitions from a yellowish core to a slightly redder, fainter outer halo, suggesting that the core is made up of older, redder stars. The outer regions are more spread out, with light smoothly decreasing in intensity, suggesting little or no current star formation. No signs of significant tidal disturbances or ongoing mergers are immediately apparent, though a possible minor disturbance can't be ruled out due to the faintness of the outer regions.