The observed galaxy presents as a relatively small, disk-shaped object. The color distribution suggests a distinct structure with a central region displaying a blue hue, potentially indicative of younger stellar populations. Surrounding this central region is a more extended area that transitions to a greener shade, suggesting a mix of stellar populations, possibly older stars or regions with ongoing star formation. A thin, reddish rim is apparent along the outer edges, which may indicate dust lanes or older stellar populations.

There appears to be a morphological disturbance present. The galaxy's light distribution is not entirely uniform, and there's a slight asymmetry in the shape. This could imply a past or ongoing interaction with another galaxy, or internal dynamic processes causing distortions in the disk. However, this may be an artifact of the image itself. Overall, while appearing mostly smooth, closer inspection reveals subtle features indicative of dynamic processes within the galaxy.
