The galaxy appears as a somewhat diffuse, elliptical-like structure. It exhibits a concentrated central region that gradually fades into a less defined outer halo. The core appears yellowish in color, potentially indicating an older stellar population. The outer regions show hints of a bluer hue, suggesting the presence of younger, hotter stars, although they may be a minor component. No obvious spiral arms or other distinct features are discernible. The overall morphology is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy seen at a significant distance, which leads to the lack of defined features. The smoothness of the light distribution suggests a well-mixed stellar population, indicating the galaxy has likely undergone significant evolution.
