The galaxy presents an elongated, cigar-shaped morphology. A bright, concentrated central bulge is evident, exhibiting a yellowish-orange hue suggesting an older stellar population. Emanating from this central region are fainter, somewhat diffuse extensions that appear slightly bluer, hinting at ongoing star formation in the outer regions of the galaxy. Overall, the galaxy appears relatively smooth in structure, with no obvious signs of major mergers or tidal disturbances, though minor disturbances can't be ruled out. The colors suggest a mix of stellar populations, with the bulge dominated by older, redder stars and the outer disk showing evidence of younger, bluer stars.
