The galaxy presents as a generally smooth, rounded structure with a concentrated central region exhibiting a yellowish-white hue. There is very little apparent texture or distinct structural features within the central region.  A slight elongation or distortion is observable, although its overall morphology is fairly regular. The outer regions appear fainter and bluer, indicating the potential presence of younger stellar populations or ongoing star formation, although the image quality limits detailed analysis of these outer areas. No obvious signs of major merging events or tidal disturbances are readily apparent.
