The galaxy presents as an elongated, cigar-shaped structure, likely a disk galaxy viewed at a high inclination. A prominent central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions of the disk are bluer, potentially indicative of ongoing or recent star formation. The galaxy appears relatively smooth, with limited evidence of distinct spiral arm structure. There may be a minor disturbance in the structure. The galaxy's morphology is suggestive of a system that has undergone some degree of dynamical evolution, possibly through interactions or mergers, resulting in its somewhat irregular shape.
