The galaxy presents as a relatively compact object, exhibiting a centrally concentrated light profile. The core region appears bright and unresolved, with a gradual fading of intensity towards the outer regions. The overall morphology suggests a smooth distribution of light, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The elongation is not very extreme, but can be observed. The color seems to trend towards the blue-end of the spectrum. 

The object's apparent size is relatively small, indicating a physically compact structure or a substantial distance. While a detailed analysis would require higher resolution data, the visual impression is consistent with an elliptical galaxy, possibly at a relatively high redshift. There is no obvious sign of active star formation regions, mergers or tidal disturbances.
