The galaxy presents as a system with a dominant central bulge surrounded by a fainter, less defined disk. The central bulge exhibits a yellowish hue, indicative of an older stellar population. The outer disk shows some subtle features, but it's difficult to resolve any spiral arm structure or distinct star-forming regions. There is a nearby smaller object that appears to be interacting gravitationally with the larger galaxy, and may be in the process of merging. Overall, the galaxy appears to be a massive system with possible evidence of ongoing or recent mergers which have disturbed the shape of the disk.
