The galaxy presents as a centrally concentrated, relatively smooth object with minimal discernible features. The morphology is largely elliptical, exhibiting a high degree of roundness. A slight color gradient is observed, with the central region appearing more yellow and the outer regions showing hints of redder hues. There is no strong evidence of spiral arms or a prominent disk component. The galaxy does not appear to be undergoing a major merging event, though minor disturbances can't be ruled out. Based on the colors, it seems to be largely composed of older stellar populations, though there could be some star formation activity.
