The galaxy appears as a centrally concentrated, smooth object with an elliptical morphology. Its core exhibits a bright, yellowish-white color, indicating a potential population of older stars. The outer regions of the galaxy display a faint, bluish halo, suggesting the presence of a younger stellar population and ongoing star formation, albeit at a relatively low rate. There is no visual evidence of strong spiral arm structures or bar features. The overall roundness indicates the galaxy is likely an elliptical or S0 type galaxy. There are no signs of major mergers or tidal disturbances.