The galaxy presents as an elliptical form, elongated significantly along its major axis. The central bulge appears bright and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. Moving outward from the core, the galaxy's light gradually diminishes. Faint blue tinges hint at the presence of younger, star-forming regions, although these are not prominent, implying a relatively low rate of star formation. No distinct spiral arm structures are discernible. The galaxy appears mostly smooth, with little evidence of major disturbances or ongoing mergers.
