The galaxy presents as a flattened spheroid with a discernible, though not sharply defined, central bulge. Its overall morphology appears relatively smooth, with minimal evidence of strong spiral arm structures or other prominent features within the disk.

The color profile suggests a significant population of older stars, indicated by the reddish-orange hue, particularly concentrated within the bulge. There is subtle color variation across the galaxy, hinting at the possibility of some ongoing, though limited, star formation activity within the disk region. The galaxy exhibits an intermediate axis ratio, appearing neither perfectly spherical nor extremely elongated. There is little to no presence of tidal tails, strong distortions, or other hallmarks of recent major merger events. Faint hints of possible minor disturbances can not be ruled out.
