The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, diffuse central region, with a gradual decrease in luminosity towards the outer edges. There are hints of a disk-like structure, but no well-defined spiral arms are visible. The color profile suggests a population of older stars, with a slightly bluer tint towards the edges, possibly indicating some ongoing, albeit weak, star formation in those regions. There is no strong evidence of any major merger events or significant disturbances to its overall structure. The galaxy appears relatively isolated, with no obvious signs of interaction with nearby galaxies.
