The galaxy presents a predominantly smooth, elliptical morphology. It appears largely spheroidal in shape, exhibiting a high degree of central concentration. There is a notable lack of discernible spiral arm structure or prominent dust lanes. The galaxy core exhibits a bright, concentrated luminosity, suggesting a significant stellar density. A color gradient is observed, with the central region displaying a yellowish-orange hue, transitioning to a slightly bluer tone in the outer regions. This color shift may indicate varying stellar populations and ages, with older, redder stars dominating the core and a younger, bluer population in the outskirts. Minor asymmetries or irregularities in the outer halo may be present, though the resolution makes these difficult to definitively classify. The overall appearance suggests a relatively evolved galaxy, potentially undergoing passive evolution. The absence of strong blue emission implies a comparatively low rate of on-going star formation activity. The angular size suggests that this galaxy is fairly distant. 
