The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a bright, concentrated luminosity, which could suggest a significant stellar density and/or active galactic nucleus. The color profile appears predominantly bluish-white toward the center, transitioning to redder hues at the outer edges, this suggests a potential variation in stellar populations with the central core housing relatively younger, hotter stars, while the periphery contains older, cooler stars. The structure appears generally smooth, with limited evidence of spiral arms or significant dust lanes. There are hints of faint extensions or disturbances at the extreme edges, but they are not prominent and their nature is uncertain. The overall morphology hints towards that of an elliptical, rather than a spiral galaxy, although a highly inclined disk galaxy cannot be excluded.
