The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth, round morphology. It presents a concentrated central region that gradually fades into its outer edges. The light distribution suggests a lack of significant internal structure, such as spiral arms or prominent dust lanes. The galaxy exhibits a color profile ranging from yellow to white, with a red shift of z= 0.223365, indicating a considerable distance from our vantage point. The light emitted suggests an older stellar population, with a low rate of ongoing star formation.
