The galaxy presents as a somewhat elliptical structure with a concentrated, bright central bulge. The luminosity appears to decrease gradually towards the outer edges, showing a smooth transition, but some features might be present. The color profile suggests a dominant population of older stars, evidenced by the yellow-orange hue, particularly concentrated in the core. There might be a hint of bluer tones towards the outer edges. The overall morphology indicates that this galaxy is likely a relatively evolved system. Some distortion in the shape cannot be ruled out from the image, but it seems to present no major disturbances.
