The galaxy presents a primarily smooth morphology. Its shape is generally elliptical, appearing moderately flattened rather than perfectly spherical or highly elongated.  There is no prominent central bulge or spiral arm structure discernible. The galaxy exhibits a color gradient, appearing bluer towards the center and becoming redder in the outer regions. This suggests a potential decline in star formation activity from the core towards the halo. No signs of any major mergers or tidal disturbances are visually apparent, although minor asymmetries cannot be ruled out.
