The galaxy presents an elongated, cigar-shaped morphology. A central bulge is evident, exhibiting a concentrated, yellowish-orange hue, suggestive of an older stellar population. Fainter, bluer extensions are observed emanating from the central region, indicating the presence of a relatively faint disk. The disk appears somewhat asymmetrical, possibly indicative of past minor interactions. There is an apparent lack of well-defined spiral arms within the disk. The overall structure suggests a transitioning morphology, not definitively elliptical nor spiral, but rather something in between, with a relatively smooth appearance. The galaxy does not exhibit any obvious signs of active merging or major disturbances.
