This galaxy presents as a largely smooth, elliptical system with a concentrated central bulge. The light profile appears to gradually diminish from the core outwards, suggesting an absence of prominent spiral arms or distinct disk features. The color index indicates a likely older stellar population, possibly with a lower rate of active star formation, supported by the redder hue of the light emitted from the system. There is a slight elongation to the galaxy's shape, deviating from a perfect sphere, but no obvious signs of major tidal disturbances or ongoing mergers are apparent in this image. The overall structure suggests a mature galaxy that has likely undergone significant morphological evolution.
