The observed galaxy presents as an elliptical morphology, although some disk features can be observed. It exhibits a central bulge, appearing as a concentrated region of relatively uniform, yellowish light. Extending outward from the bulge is a fainter, somewhat flattened disk. This disk does not exhibit well-defined spiral arm structures, but rather appears as a more diffuse distribution of light. A slight tilt is observable relative to our line of sight. The disk appears more extended along its major axis than its minor axis. There is some indication of minor irregularities or disturbances in the disk structure. The overall color of the galaxy indicates a moderate amount of ongoing star formation.
