The galaxy presents a generally smooth morphology, with a slight elongation, appearing more like a flattened spheroid than a clear spiral or irregular type. Its color index suggests a relatively evolved stellar population. The galaxy's profile exhibits a centrally concentrated brightness that fades gradually outwards with no strong indication of significant star formation. There is no significant disk structure or spiral arms. The overall appearance is consistent with an elliptical galaxy at moderate redshift, showing no evidence of recent or ongoing major mergers, although there might be minor disturbances present.
