This galaxy exhibits a distinctly elongated, cigar-like morphology. The light distribution appears smooth, suggesting a lack of prominent spiral arms or irregular features. A central bulge is visible, displaying a yellow-orange hue that indicates an older stellar population. The outer regions fade into a bluish color, suggesting the presence of some younger, hotter stars, although not in significant quantities to form a disk. There is no apparent evidence of significant merging or tidal disturbances in the immediate vicinity. The galaxy has a high probability of being a smooth galaxy.
