The galaxy exhibits a predominantly smooth morphology, with a notable central bulge. The overall shape appears roughly round, displaying a slight ellipticity. There is evidence of some features or disks, but they are not the dominant characteristic. The galaxy demonstrates a color gradient, with the central region appearing more yellow, possibly indicating an older stellar population and/or significant dust obscuration. Fainter, bluer regions surround the core, suggesting recent star formation activity. No major mergers or significant tidal disturbances are apparent, although a minor disturbance is not entirely ruled out. The galaxy demonstrates ongoing star formation with a specific star formation rate range implying it is an active galaxy.
