This galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, with a yellowish-white hue suggesting an older stellar population. Fainter, less defined regions of bluish light extending from the central bulge imply the possibility of some younger stars and ongoing or recent star formation. There is no obvious spiral arm structure. The galaxy exhibits an approximately circular morphology, showing no signs of strong tidal disturbances or ongoing mergers, although subtle irregularities might be present upon closer inspection. The overall color index suggests that this galaxy is dominated by evolved stars, but with pockets of younger, bluer stars present.
