The galaxy exhibits a generally smooth morphology, appearing largely featureless across its structure. The light distribution suggests an elongated, cigar-like shape. There is a concentration of bluer light towards the center of the galaxy which fades towards the edges. The outer regions of the galaxy appear less defined and more diffuse, indicating a gradual decline in stellar density with increasing radial distance. The galaxy shows no visual signs of significant tidal disturbances or ongoing mergers, but there are some minor disturbances. 