The galaxy presents a primarily smooth morphology, appearing as an elliptical or lenticular type when viewed at this resolution. Its shape is elongated, exhibiting an axis ratio suggesting it is not perfectly face-on. The color profile indicates an older stellar population dominates, evidenced by a yellow-orange hue in the central bulge region. A subtle greenish tint toward the outer regions suggests a small amount of ongoing star formation, or potentially a population of younger, bluer stars present in the disk or outer regions, though the overall star formation rate appears low. No significant tidal disturbances or signs of recent mergers are immediately apparent. There might be a very slight asymmetry indicating a minor gravitational interaction, but the overall structure appears relatively undisturbed and relaxed.
