The galaxy presents as a disk galaxy, observed at a high inclination. It exhibits a slightly elongated, cigar-like shape. There appears to be a central bulge region, brighter and more concentrated, indicative of a higher stellar density. The disk component is less defined, with a smoother, almost featureless appearance. The colour profile suggests an aging stellar population, with a yellowish-red hue dominating the galaxy's light. There is no visually prominent spiral arm structure or active star-forming regions discernible. No major distortions or tidal features are evident, suggesting the absence of recent major merger events. The galaxy seems to be relatively isolated and undisturbed.
