The galaxy presents as a generally smooth, elongated structure with a cigar-like shape. The central region appears to exhibit a higher concentration of luminosity, suggesting a possible bulge or core. A slight gradient in color is visible, with the central region trending towards a yellowish-white hue, potentially indicating an older stellar population. The outer regions fade in intensity, exhibiting a bluer tint.

The galaxy's elongated form implies it is being observed at a high inclination. No distinct spiral arms or bar structures are readily apparent, consistent with a potentially lenticular or early-type spiral morphology. There appears to be very slight disturbance in the form of a tail or smaller secondary structure at the lower right of the center of the galaxy.

Based on its overall appearance, this galaxy appears to be a relatively massive galaxy undergoing active star formation.
