The galaxy presents as a relatively smooth, elliptical object. Its core appears luminous with a yellowish hue, suggesting a population of older stars. The light gradually fades towards the outer regions, which appear to be less active in star formation. There is no clear disk structure or spiral arms visible, indicating a lack of significant ordered rotation or ongoing major mergers. There appear to be no major disturbances. The morphology suggests the galaxy is at an advanced stage of its evolution.
