The galaxy appears to be a relatively luminous, early-type system, exhibiting a generally smooth morphology. The light distribution is centrally concentrated, with a near-circular overall shape but is slightly elongated. There is some evidence of tidal disturbances or ongoing interactions, as it looks like it may be merging with another nearby galaxy. The red color suggests that the galaxy is dominated by an older stellar population and that there may be a low rate of star formation.
