The galaxy presents as a spiral, observed at an angle somewhere between face-on and edge-on, closer to face-on. The nucleus appears as a moderately sized central bulge, not particularly dominant. Some evidence of a disk is apparent, with indications of spiral arms, but they are not very well defined. There is some indication of a possible bar structure, but it is not particularly prominent, perhaps weak. No major mergers are occurring. Evidence suggests moderate star formation.
