The galaxy presents an overall elliptical morphology, with a smooth, relatively featureless appearance. The central region exhibits a bright, concentrated core, suggesting a significant concentration of stars. The light distribution appears to fall off gradually from the center outwards, with no distinct spiral arms or bar structures visible. There is a slight elongation to the galaxy's shape, hinting at a possible transition from a perfectly spherical shape. The color profile reveals a predominantly yellowish-red hue in the central bulge, indicative of an older stellar population. Fainter, bluer tones are observed in the outer regions, possibly reflecting the presence of younger, hotter stars or ongoing star formation, albeit at a low rate. No significant signs of tidal disturbances, mergers, or active galactic nuclei are readily apparent in the image.
