This galaxy appears to be a spiral type, although the arms are not clearly defined in the image. It exhibits a moderately bright central bulge, which suggests the presence of a supermassive black hole in the center. The color gradient from the center outwards shows a transition from a yellowish hue in the central bulge to a bluer tint in the outer regions. This may indicate that star formation is more prevalent in the outer parts of the galaxy. I would estimate the physical size of the galaxy to be around a few kiloparsecs across, given the radial distribution of light observed. There may be interaction with a nearby object, which suggests possible merging activity, or perhaps just some minor tidal disturbances. The star formation rate seems relatively low, but not quite quiescent.
