The galaxy presents as an elongated, cigar-shaped structure. There is a smooth light distribution across the galaxy, with the central region appearing slightly more concentrated. The colour profile suggests a population of older stars, with a yellowish hue dominating the central bulge and disc. The galaxy has a relatively undisturbed morphology, exhibiting no obvious signs of ongoing major mergers or tidal interactions. However, there may be some signs of minor disturbance on one side. The galaxy appears to be relatively isolated.
