The object appears to be a spiral galaxy, likely seen from a considerable distance. It is characterized by a diffuse, somewhat asymmetrical structure. The central region presents a slightly brighter, yet not sharply defined, core. Spiral arms are visible, though not distinctly delineated. These arms appear to be somewhat fragmented, with a patchy distribution of luminosity.

The galaxy exhibits a general bluish hue overall, suggestive of ongoing star formation. There is a faint tidal stream or extended halo of material extending from one side of the galaxy. The structure is clearly not a smooth elliptical. The morphological classification favors a spiral type with some level of disturbance or recent interaction.
