This galaxy exhibits a distinct, elongated morphology. The primary structure appears to be a prolate spheroid with a cigar-like shape. A central bulge is visible, emitting a primarily yellow-orange hue, suggestive of an older stellar population, with diminished star formation activity. The galaxy shows evidence of some degree of disk-like structure, albeit not as clearly defined as in spiral galaxies. A faint disk appears to extend around the bulge. There is also a slightly irregular or disturbed shape, possibly due to a past minor gravitational interaction. Patches of blue light are visible in the bottom left, implying regions of more recent, ongoing star formation, although these areas are not particularly prominent. Overall, the galaxy presents characteristics intermediate between a pure elliptical and a spiral system, potentially representative of a lenticular galaxy undergoing interactions.
