Observed at Right Ascension 96.74 degrees and Declination -51.32 degrees, this galaxy presents as a relatively faint object, possibly a high-redshift system. Morphologically, the galaxy exhibits features suggestive of a potential ongoing interaction or merger. There appears to be some distortion in its overall shape, with elongated features.

A degree of asymmetry is noticeable in the light distribution. I cannot assess the presence of any spiral arm structure, but there appears to be some clumpy structures. The core of the galaxy appears as a relatively smooth, centrally condensed region. Color variations across the galaxy are subtle. Further spectral analysis is needed to determine the nature of these features and confirm the nature and distance of this galaxy.
