The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a generally rounded morphology, with minimal evidence of a disk structure or spiral arms. There is a slight elongation but it does not appear cigar-shaped. The galaxy's color suggests an older stellar population, which may be reflected in the apparent lack of star formation. There is no strong evidence for ongoing major mergers or significant tidal disturbances within the visible structure. A very slight color gradient from the center to the outskirts may suggest differing stellar populations.
