The galaxy exhibits a generally smooth morphology with some visible features, appearing as a flattened spheroid. Its shape is elongated, with an axis ratio suggesting it is not a face-on spiral, but rather viewed at an angle.

The central region of the galaxy is concentrated and brighter in the observed optical bands, hinting at a possible bulge. There appears to be a more diffuse, fainter halo or disk component surrounding the core.

The color gradient is relatively subtle. The central bulge appears slightly redder compared to the outer regions, which exhibit a bluer hue. This color difference could imply variations in stellar populations or dust content within the galaxy, with the center potentially hosting older, redder stars, and the outer regions exhibiting ongoing or more recent star formation.

No strong tidal features or signs of recent mergers are immediately apparent in this image. The overall appearance suggests a relatively undisturbed system, without significant morphological distortions.
