This galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, exhibiting a radial decrease in luminosity from its core. The core appears bright and somewhat unresolved, suggesting a dense stellar population or possible active galactic nucleus.

The galaxy displays a subtle color gradient. The central regions appear more yellow/white, possibly indicative of an older stellar population. Fainter bluish hues are visible in the outer regions of the galaxy, which could suggest younger stars or some ongoing, though limited, star formation. There is no distinct disk structure or spiral arm pattern visible. There are some minor asymmetries or disturbances, but no clear evidence of a recent major merger event.
