This galaxy presents a flattened, disc-like morphology. The central region exhibits a high surface brightness, appearing almost unresolved and intensely luminous. Surrounding this bright core is a more diffuse, extended halo. A faint, yet discernible spiral structure can be observed emanating from the central bulge. This indicates an active star-forming region. There is a slightly blue color in the disk, particularly at its outer edges, which is indicative of recent or ongoing star formation. The overall color index suggests the presence of both young, hot stars and older stellar populations within the galaxy. Additionally, there appears to be some minor disruption in the disc which can be a possible sign of merger activity, and a significant fraction of its light is concentrated towards the center, suggesting the presence of a bulge component.
