The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a concentrated, bright luminosity, suggestive of a significant stellar population or active galactic nucleus. Fainter, diffuse light extends outwards from the central region, indicating a stellar halo or disk. Evidence of spiral arm structures or distinct features are not readily apparent. The overall color appears yellowish-red, potentially indicating an older stellar population or significant dust obscuration. There is no clear evidence of ongoing major merging activity, though minor tidal disturbances cannot be ruled out.
