This galaxy appears to be a relatively compact object. Its morphology suggests it is likely an elliptical galaxy. The galaxy exhibits a smooth and centrally concentrated light distribution. There is a slight elongation, possibly indicating a transition between spherical and more cigar-shaped ellipticals. There are hints of a yellowish or orange hue in the galaxy's core, which could indicate an older stellar population and relatively low ongoing star formation. There is no indication of significant tidal disturbances, merging activity, or prominent spiral arm structures. The overall visual impression is that of a passively evolving galaxy.
