The galaxy presents a primarily smooth morphology, with a slightly elongated, cigar-shaped appearance. The central bulge exhibits a concentrated, bright, yellowish-white luminosity, suggesting an older stellar population. Surrounding the bulge, a fainter, bluish-white disk is observed, indicating the presence of younger stars and possibly ongoing star formation. There appears to be a minor asymmetry or disturbance in the outer regions of the disk, though no major mergers or interactions are immediately evident. The galaxy exhibits a disk-like structure, but the dominance of the smooth central bulge suggests a classification leaning towards an intermediate type, possibly between a spiral and an elliptical galaxy.
