This galaxy presents as a spiral type, exhibiting a prominent, moderately sized central bulge. The disk structure is clearly visible and oriented at an oblique angle to our line of sight. Within the disk, distinct spiral arms are observed, generally wound in a medium configuration. Evidence suggests the presence of two dominant spiral arms. The central bulge appears yellowish-white, suggesting a population of older stars, while the spiral arms exhibit a bluer hue, indicative of ongoing star formation. No obvious signs of a major ongoing merger event are apparent; however, the galaxy does show minor signs of disturbance within the spiral arms, potentially indicating a past interaction. A bar structure is observed that is not very prominent.
