The galaxy presents a morphology consistent with a lenticular or early-type spiral galaxy at a moderate redshift. It appears as a diffuse, centrally concentrated object with a relatively smooth light distribution. There is no distinct spiral arm structure visible, and the overall color is relatively uniform, suggesting an older stellar population. The galaxy exhibits an elliptical shape with a hint of a possible disk component seen edge-on. There is no evidence of ongoing major mergers or tidal disturbances. The galaxy's light profile indicates a substantial bulge component, and the absence of strong blue colors suggests low current star formation activity.
