The galaxy presents as an elongated structure with a noticeable central bulge. The color gradient transitions from a yellowish-white core to fainter, bluish hues at the outer edges, indicating a possible mix of stellar populations, with older stars concentrated centrally and younger, hotter stars in the outer regions. There appears to be a faint disk-like component oriented roughly along the major axis. The edges of the galaxy are somewhat indistinct, suggesting a gradual decrease in stellar density with increasing distance from the center, possibly surrounded by a faint halo. There's a slight asymmetry in the overall shape, with a more pronounced extension towards one end, which could indicate tidal interactions or an ongoing merger event, though no obvious companion galaxy is visible in the immediate vicinity. Evidence of dust lanes is subtle but visible in the disk.
