This galaxy exhibits a relatively smooth, featureless morphology, suggesting it is likely an elliptical galaxy. It appears somewhat elongated, possessing an axis ratio that deviates slightly from a perfect circle. There are no clear signs of spiral arms or a prominent disk structure. The galaxy's color is generally redder compared to typical spiral galaxies, indicative of an older stellar population with lower ongoing star formation. No significant signs of tidal disturbances or ongoing mergers are apparent, although minor disturbances cannot be ruled out at this resolution. Overall, the galaxy seems to be a relatively quiescent system.
