The galaxy presents a largely smooth morphology, indicating an elliptical or lenticular classification. It appears nearly circular in projection on the sky, showing no significant elongation. There is a slight color gradient, with a yellowish-orange hue concentrated towards the galactic center. No distinct spiral arm structures or prominent dust lanes are discernible. The overall light distribution suggests a relatively evolved stellar population, consistent with a passive galaxy dominated by older stars. Indications of minor disturbances suggest a past or ongoing interaction, though major mergers or strong tidal features are absent. There is no notable presence of bright blue star-forming regions, reinforcing the likelihood of low current star formation.
