The galaxy presents as an elongated, somewhat cigar-shaped structure. The central region appears brighter and more concentrated, possibly indicating a higher density of stars within the galactic nucleus. The galaxy exhibits a relatively smooth texture, with little evidence of distinct spiral arms or prominent dust lanes. There is a subtle color gradient, with a slightly bluer hue towards the edges and a yellower tone in the center. This color variation suggests that the outer regions may contain populations of younger, hotter stars, while the central region is dominated by older, cooler stars. Overall, the galaxy gives the impression of being relatively mature and evolved. Evidence of a past or ongoing minor disturbance to its structure is possibly noted.
