The galaxy presents as a generally smooth, elliptical morphology, though with some subtle deviations from perfect sphericity. It displays a concentrated central bulge that graduates outwards. The central region exhibits a yellowish-white color, potentially indicative of an older stellar population dominating this area. The outer regions appear slightly bluer in hue. There is minimal evidence of significant spiral arm structure. The overall light distribution suggests a relatively relaxed system, lacking prominent features such as tidal tails or strong signs of recent merger events. Based on the estimated distance to the object, we can infer a substantial size.
