The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse light profile. Its color appears to be redder, suggesting an older stellar population dominated by evolved stars and reduced ongoing star formation. There's no clear evidence of spiral arms or a distinct disk component from this perspective. The overall shape is relatively round, exhibiting minimal elongation or tidal disturbances. No signs of recent major merger events or significant morphological disruptions are immediately visible in the image. The light is fairly even, with a slight concentration at the center, but there is no evidence of an extremely bright, active galactic nucleus.
