The galaxy appears as a luminous object, exhibiting a somewhat elliptical morphology. A dominant, relatively smooth and centrally concentrated bulge structure is observed, characterized by a yellowish hue. This suggests an older stellar population within the bulge. Adjacent to the main bulge, a smaller, distinct region displays a bluer color, potentially indicating ongoing star formation. Although there appears to be two separate objects, they may be in the process of merging. No prominent spiral arm structure is readily apparent. The galaxy has a redshift of approximately 0.205, indicating its considerable distance.
