The galaxy exhibits a largely smooth morphology, with a predominantly round shape. It appears to have a concentrated central bulge that is colored yellow, indicating an older stellar population. The outer regions are more diffuse and appear to contain a mix of light possibly from ongoing or recent star formation. There is little evidence of spiral arm structure or significant dust lanes. The galaxy does not seem to be undergoing any major mergers, although there might be some minor gravitational disturbances visible in the outskirts.
