The galaxy presents as an elongated, cigar-shaped structure. It has a relatively smooth appearance with only slight variations in brightness across its body. There is a suggestion of a disk-like component, though not sharply defined, with what appear to be faint arms or spiral segments. The color is predominantly bluish-white suggesting a younger stellar population. There is little evidence of ongoing major star formation activity. There does not appear to be a significant dust lane visible. The galaxy appears isolated, with no obvious signs of tidal disturbances or interaction with neighboring galaxies. The overall morphology suggests a galaxy in the transition phase, potentially evolving from a spiral toward a more quiescent elliptical form.
