The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution that suggests an older stellar population dominating its overall appearance. The central region appears brighter and more concentrated, indicating a possible bulge. The color profile shows a blue-white hue. The galaxy's shape is largely rounded, showing little evidence of significant rotational flattening or a distinct disk component. There is some minor asymmetry potentially caused by a minor disturbance. It appears to be a relatively isolated system, with no obvious signs of major mergers. Overall, it is a low mass system, with low star formation. 
