The galaxy presents as an elongated, cigar-shaped structure with a prominent central bulge. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the bulge, a fainter, more diffuse disk is observed. This disk appears less structured, with only subtle hints of spiral arm features. There may be areas of active star formation within the galaxy, but they are not immediately apparent. Overall, the galaxy exhibits a smooth appearance. There appears to be an object close to the galaxy, which might be undergoing merging or may just be a close object in the foreground or background.
