The galaxy in question appears as a diffuse object, approximately circular, with a centrally concentrated luminosity profile. The core region exhibits a notable redder hue compared to the outer parts. The galaxy demonstrates a relatively smooth texture with no obvious spiral arms. A slight asymmetry is observable, indicating the possibility of a minor interaction or disturbance. There is a notable absence of well-defined features, and no signs of a strong bar structure. The object has a distinct morphology with some texture.
