The galaxy appears to be a relatively smooth, elliptical galaxy with a near-spherical morphology. It exhibits a concentrated central bulge that dominates its overall light profile. There is no discernible disk structure or spiral arms. Minor disturbances may be present, but there does not appear to be evidence of ongoing major mergers or tidal interactions. The galaxy presents a redder color, indicating a population of older stars with relatively low ongoing star formation. It appears to have a relatively high mass.
