The galaxy presents a generally smooth and rounded appearance. It exhibits a concentrated central region with a yellowish hue, suggesting an older stellar population. There are no clearly defined spiral arms or bar structures visible. Faint, diffuse extensions or tidal features appear to be present. The extensions are characterized by a blueish tint, indicating the presence of younger stars. Based on color indices and redshift, this galaxy likely has a substantial stellar mass and a relatively low star formation rate. The lack of significant morphological disturbances suggests that it is not currently undergoing a major merging event, but minor disturbances may be present.
