This galaxy appears to exhibit a largely spheroidal morphology, with a smooth overall light distribution. It is moderately luminous, with a predominantly reddish-yellow hue, suggesting an older stellar population with relatively little ongoing star formation. The galaxy does not exhibit a clear disk structure, and instead appears as a concentrated central bulge. There are some signs of potential tidal disturbances or merging activity in the form of extended or asymmetric features, although these features are not particularly pronounced. Close inspection reveals that the central portion of the galaxy is slightly more intense than the surrounding regions. Based on its appearance, it could be classified as an elliptical galaxy possibly undergoing or having undergone a minor merger.
