The galaxy appears to be a luminous elliptical galaxy. It exhibits a generally smooth morphology, with no obvious spiral arms or a prominent disk structure visible. The light profile suggests a high degree of central concentration, with the brightest emission emanating from the core region.

The galaxy's color is predominantly yellow-orange, indicating a relatively old stellar population with a lower proportion of young, massive stars. The galaxy displays a well-defined spheroidal shape, appearing nearly circular in projection, with only a slight deviation from perfect roundness. There is no strong evidence of recent or ongoing major merger events, although there might be some minor disturbances that cannot be resolved at this image resolution.
