The galaxy appears to be an elliptical or lenticular type, exhibiting a largely smooth and centrally concentrated light distribution. Its shape is predominantly in between a round and cigar shape, displaying a somewhat elongated form. There is a suggestion of a possible minor disturbance or interaction occurring, as subtle asymmetry or irregularity in the light distribution is apparent. This object does not have a pronounced spiral arm structure. The central region is bright, indicating a high concentration of stars. Given its estimated size and redshift, this is a galaxy located at a considerable distance, characterized by moderate star formation activity and a stellar mass within a substantial range.
