The galaxy appears to be a relatively small, faint, elongated system. It presents a smooth, featureless morphology, lacking prominent spiral arms or a distinct central bulge. The light is dominated by a bluish hue, suggesting the presence of a population of hot, young stars, although this is subtle. The galaxy exhibits a flattened, cigar-like shape. There is no obvious indication of ongoing major mergers or tidal disturbances, though minor disturbances or interactions cannot be ruled out completely at this resolution. The observed morphology suggests a system that may be transitioning or represents a later stage in its evolution.