The galaxy presents an elliptical morphology with a moderate redshift, indicated by its relatively faint g-band magnitude compared to its r-band magnitude. The core exhibits a diffuse and somewhat irregular structure. There is evidence of a possible tidal tail or stream extending from the main body of the galaxy, suggesting a past or ongoing interaction. The redder color in the core indicates an older stellar population with a decreased presence of ongoing star formation. The outer regions of the galaxy appear fainter and more diffuse, suggesting a decrease in stellar density with increasing radius. The overall light distribution implies a system with a relatively low concentration. Minor disturbances or irregularities hint at a dynamically active history.
