The galaxy appears to be a relatively compact object with a smooth, elliptical morphology. There is minimal evidence of spiral arms or a well-defined disk structure. The light distribution suggests a centrally concentrated stellar population, with the intensity gradually decreasing towards the outer regions. It presents a fairly round shape. The color profile indicates a relatively evolved stellar population, with a color consistent with older stars. There may be evidence of a minor interaction or disturbance, but it looks to be a single structure, not the result of a recent major merger. Overall, the galaxy is likely a relatively massive elliptical galaxy at a moderate redshift, showing a low rate of star formation.
