The galaxy presents as an elongated structure. Its color profile is dominated by warmer tones, indicating a population of older stars and reduced star formation relative to bluer galaxies. The galaxy exhibits a smooth morphology, showing little evidence of spiral arms or significant dust lanes. The shape of the galaxy is cigar-like, strongly suggesting it is an elliptical galaxy, or potentially a lenticular galaxy seen edge-on. Evident from the somewhat disturbed structure, the galaxy could be undergoing a minor merger with another galaxy or experiencing some form of gravitational interaction. No clear signs of strong tidal tails or prominent merger remnants are observable.
