The galaxy appears as a flattened, elongated structure, exhibiting characteristics of a disk galaxy viewed edge-on. The central region shows a brighter, concentrated luminosity, possibly indicating the presence of a bulge. The overall color suggests a population of older stars, potentially with ongoing star formation, but likely at a subdued rate. There is limited evidence of spiral arm structure; the disk seems relatively smooth. The galaxy presents with only minor signs of disturbance, with a high probability that it is not currently undergoing any significant merger activity. Its shape is more closely akin to a cigar, than that of a round structure.
