The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution is centrally peaked with a gradual falloff in surface brightness with increasing radius. There is a slight elongation, but overall the shape is approximately circular. The color appears to be moderately red, suggesting an older stellar population and a lack of significant ongoing star formation. There is no evidence of spiral arms, dust lanes, or other prominent features typically associated with actively star-forming disk galaxies. There is no apparent sign of interactions or mergers.
