The galaxy presents as an elongated, somewhat cigar-shaped structure. The central region exhibits a bright, concentrated luminosity, indicating a significant stellar population and/or possible active galactic nucleus. Moving outward from the center, the light appears to diffuse into a less concentrated, disk-like structure. There is a hint of spiral arm structure, appearing somewhat disrupted or flocculent, with some bluish regions, which could be areas of active star formation. The overall color profile suggests a mix of older stellar populations in the central bulge, and younger stars and dust in the outer disk. There is no evidence of major tidal disturbances or ongoing mergers, although some minor asymmetries may be present.
