The galaxy presents a primarily smooth morphology, appearing as a lenticular or early-type spiral galaxy at a moderate redshift. There is a slight elongation in its shape, but it largely appears rounded. The light distribution suggests a central bulge, gradually fading outward without distinct spiral arm structures. A subtle color gradient is visible, shifting from slightly bluer hues in the central regions to redder tones in the outer regions. This could be indicative of a younger stellar population in the core or a presence of a weak active galactic nucleus. There are minimal signs of significant disturbances or recent merger activity, with only a slight asymmetry suggesting a possible minor interaction. The galaxy exhibits a relatively compact structure, and its overall appearance indicates a relatively quiescent evolutionary state.
