The galaxy appears to be a disk galaxy, viewed at a relatively high inclination. It exhibits a bright, concentrated central bulge region, with evidence of a flattened, extended disk component. The color gradient suggests a population of younger, bluer stars in the disk, transitioning to redder, older stars in the bulge. There is a notable level of disturbance or asymmetry within the disk structure, with indications of possible tidal features or minor distortions suggestive of an interaction with another galaxy. These features are primarily localized to one side of the galaxy. The presence of green color indicates some ionized gas in the region, possibly associated with star formation.
