The galaxy presents as a largely smooth, elliptical-like structure with a concentrated, bright central bulge. A slight yellowish hue is prominent, suggesting an older stellar population. There is a very faint disk around the central bulge, but it isn't clearly defined. There does not appear to be any significant ongoing merger activity or major disturbances present, though faint extensions hint at minor interactions. It's generally circular in form. Based on the high central concentration and the lack of well-defined spiral arms or prominent dust lanes, this galaxy is likely an early-type galaxy, possibly an elliptical or lenticular type. The color indicates a lack of significant current star formation.
