The galaxy presents a somewhat elliptical morphology, appearing flattened. Its color profile indicates a dominant redder hue concentrated towards the central regions, suggesting an older stellar population. There is a brighter core with extended diffuse emission around it. The relative smoothness of the light distribution suggests it could be an early-type galaxy. Although, there appears to be a subtle hint of a disk feature, but this needs further analysis due to image resolution. A possible interacting companion may be causing disturbance in the disk, but needs further inspection.
