The galaxy presents a moderately inclined disk-like structure. Its overall color profile suggests a mix of stellar populations, with a central region that appears slightly more yellow, indicative of older, less massive stars. The outer regions of the disk exhibit a bluer hue, consistent with the presence of younger, hotter stars potentially formed in recent or ongoing star formation events. The disk appears somewhat disrupted or irregular in shape, showing hints of tidal features or possible interactions with other galaxies, although no clear companion is immediately visible. There are faint extensions or diffuse structures surrounding the main body of the galaxy, potentially representing tidal debris or stellar halos. The light distribution is relatively smooth, however, the structure is somewhat fragmented, which is typical of galaxies that could be merging.
