The galaxy presents as an elongated, cigar-shaped structure, suggesting a classification toward the elliptical end of the Hubble sequence. The color distribution appears relatively uniform across the galaxy's extent, hinting at an older stellar population and suppressed star formation activity. No distinct spiral arms or prominent dust lanes are discernible. There is a slight central brightness concentration, possibly indicating the presence of a galactic nucleus. The galaxy appears relatively undisturbed, with no clear signs of ongoing major merger activity, although a slight asymmetry might suggest a past minor interaction or internal dynamical processes.
