The galaxy presents as an elongated, cigar-shaped structure, appearing approximately 3.8 kpc in diameter based on photometric measurements. The central region exhibits a yellowish hue, suggesting an older stellar population and reduced star formation activity in this area. Extending outwards from the core, the galaxy displays a more diffuse and less distinct structure. There are slight disturbances noted, although the galaxy is mostly intact. It is not perfectly smooth; the central bulge appears slightly brighter and more defined. The overall color gradient indicates a declining rate of star formation from the center outwards, implying that the younger, bluer stars are less prominent in the nuclear region.
