The galaxy presents as a highly elongated, cigar-shaped structure. Its light profile appears relatively smooth. The galaxy exhibits a clear colour gradient, shifting from bluer tones at the central region to a redder hue in the outer edges. This may indicate differences in stellar populations or dust content across the galactic body, where the centre may be host to newer or bluer stars. Overall, the galaxy appears undisturbed, without evidence of significant tidal features or ongoing major mergers.
