The galaxy appears to be an elliptical galaxy, with a smooth, largely featureless morphology. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The overall shape appears close to circular. There may be a very subtle elongation, but it is difficult to confirm. The galaxy exhibits a colour gradient, with the core appearing more red-yellow and the outer regions displaying a bluer tint. This could be due to the presence of an older stellar population in the central region and younger stars in the outer portions. There is no evidence of strong spiral arms, a bar, or any obvious signs of recent or ongoing major mergers, and minimal disturbance to the overall structure.
