The observed galaxy presents a generally smooth, elongated morphology. A central bulge is evident, characterized by higher luminosity and a more condensed structure compared to the outer regions. The light distribution is not perfectly symmetric, with a slight tapering visible on the upper portion of the galaxy. Overall, the galaxy exhibits a noticeable red color, suggesting an older stellar population with reduced ongoing star formation. There appear to be some subtle irregularities or minor disturbances present in the outer region, although it is difficult to determine the origin or nature of these features with certainty. Evidence suggests this is an elliptical galaxy. 
