The galaxy presents as a flattened elliptical or lenticular system, oriented at a steep inclination relative to our line of sight. The central bulge appears dominant, exhibiting a smooth, concentrated luminosity profile with a yellowish-orange hue, suggesting an older stellar population. Faint disk-like structure is suspected, though poorly defined. No prominent spiral arms or distinct dust lanes are discernible within the structure. Overall, it appears to be a quiescent galaxy, possibly with low ongoing star formation, at a significant distance. The shape indicates a possible cigar-shaped galaxy.