This galaxy presents as a slightly elongated, disk-like structure. The central region appears bright, possibly indicative of a dense stellar population or active galactic nucleus. The galaxy exhibits a smooth texture, with a general lack of distinct spiral arm structures or prominent dust lanes visible in this image. The color gradient transitions from a brighter, yellowish core to a dimmer, slightly bluer periphery, suggesting a possible difference in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars in the outer regions. Overall, the galaxy seems to be relatively isolated, with a possible minor disturbance visible. The image resolution is not high enough to resolve individual stars or star clusters.
