This galaxy, observed at a redshift of approximately 0.21, presents as a somewhat smooth, elliptical-like structure. The primary body is a diffuse, centrally concentrated region with a generally round shape, with slight irregularities visible, suggesting potential interactions. There is a merging component with an apparent stream or tidal tail, with a small round blob. The colour profile indicates a moderate abundance of older stars, with the bright region appearing more orange in colour and suggesting some star formation. This observed configuration may be indicative of an ongoing minor merger or tidal disruption event. The object is relatively compact, but resolved. Further spectral analysis would be beneficial to confirm the age and metallicity of the stellar populations, as well as to more conclusively determine the nature of the interaction and the morphology of the galaxy.
