The galaxy presents an elliptical morphology, though with some structural asymmetry. The central region is bright and relatively smooth, indicating a concentrated stellar population likely dominated by older stars. A fainter, elongated feature extends from this core, possibly a tidal tail or a disturbed disk resulting from an interaction. There is also evidence of possible recent merging activity. There is a strong signature of this galaxy merging with another galaxy. The colors are consistent with an intermediate redshift object. Overall, it suggests a galaxy that has experienced significant interactions.
