The galaxy presents a somewhat elongated morphology, appearing primarily blue in color. The central region displays a brighter, more concentrated luminosity, suggestive of a galactic bulge. Fainter, diffuse extensions are observed, oriented vertically, possibly indicating a flattened disk structure viewed at a moderate inclination. These extensions appear somewhat disturbed or irregular, hinting at either tidal interactions or internal activity such as star formation. There is no strong evidence of spiral arm structure discernible at this resolution. The overall form implies a galaxy of moderate size and mass, with signs of ongoing or recent star formation.
