The galaxy appears to be a lenticular or possibly an edge-on spiral galaxy, characterized by a flattened, elongated shape. The central bulge is visible but not overly prominent, exhibiting a yellowish or slightly reddish hue, suggesting a population of older stars. The disk of the galaxy appears relatively smooth and featureless, with no readily apparent spiral arm structure. There is a subtle color gradient, transitioning from the central bulge to a bluer halo or outer disk. The overall structure indicates that this galaxy is likely not currently undergoing a major merging event.
