The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The core region is relatively bright, displaying a yellowish-orange hue, potentially indicative of an older stellar population. This central region is surrounded by a less luminous, somewhat extended halo that transitions into a greenish hue. This color may imply some ongoing, although subdued, star formation, or a difference in the age and metallicity of the stars in the outer regions of the galaxy. No significant spiral arm structures or distinct dust lanes are apparent, suggesting that this galaxy is likely an elliptical or lenticular type. There is no major disturbance or evidence of on-going major merging events. Based on its relatively smooth appearance and lack of discernible features, I would classify it as a relatively undisturbed, quiescent galaxy.
