The galaxy presents as a primarily smooth, lenticular morphology, exhibiting a moderate disk-like structure. It appears elongated, suggesting a cigar-like shape rather than a perfect circular form. The central bulge is prominent and exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, bluer regions are visible along the edges of the disk. These regions imply the presence of younger, hotter stars and ongoing star formation. There is little indication of significant spiral arm structure or major disturbances, although minor disturbances in the disk cannot be completely ruled out. The galaxy is likely a quiescent system with a low star formation rate, where star formation is concentrated in the outer regions.
