The galaxy presents as a relatively smooth, disk-like structure, though with a noticeable cigar-shaped elongation along its major axis. A bright, concentrated central bulge is evident, appearing a yellow-orange hue. Fainter, bluish extensions are present on either side of the central bulge, potentially indicating the presence of spiral arms or a more extended disk component. These extensions exhibit a slightly clumpy texture. The overall morphology suggests an intermediate classification between a lenticular and spiral galaxy. There is a subtle asymmetry to the disk, with one side appearing slightly more extended or disturbed than the other, possibly indicating a minor gravitational interaction or recent accretion event. The color gradient from the bulge to the outer regions suggests a change in stellar populations, with older, redder stars dominating the bulge and younger, bluer stars residing in the disk. Star formation appears to be low.
