The galaxy presents as a somewhat amorphous, extended object with a discernible central condensation. The overall color profile suggests the presence of both older stellar populations and regions of ongoing star formation. The central region appears relatively smooth, transitioning to a more complex, textured periphery. There is a prominent, yet diffuse, ring like structure visible. Visual inspection indicates a lack of grand spiral arm structure. The galaxy appears moderately disturbed, possibly due to a minor interaction or internal processes. There are noticeable color variations and irregularities in the outer regions, suggestive of localized star formation or uneven dust distribution.
