The galaxy presents as a centrally concentrated object, ellipsoidal in shape with a smooth, diffuse appearance. The central region exhibits a bright, concentrated core, with a gradual decrease in luminosity towards the outer edges. Color gradients are subtle, with the central bulge appearing slightly more yellow/red, potentially indicating an older stellar population. The outer regions show a hint of bluer tones, possibly from younger, hotter stars, but these are faint. There is no visible dust lane or spiral arm structure. The overall morphology suggests a relatively evolved system with minimal ongoing star formation. The major axis is noticeably longer than the minor axis, with a cigar shape, but with a slight roundness, suggesting an intermediate ellipticity. There is no obvious sign of tidal interactions or mergers.
