The galaxy presents a morphology that appears neither fully smooth nor exhibiting a well-defined spiral structure, hinting at an intermediate classification. A central bulge region is evident with a high surface brightness, suggesting a concentration of older stellar populations. The overall shape appears moderately elliptical. Faint disturbances seem present in the galactic structure, possibly indicative of tidal interactions or a recent minor merger event. A small percentage of roundness is exhibited, with the galaxy appearing somewhere between a perfect sphere and a cigar shape. There is a clear sign of merging or disturbance. 