The galaxy presents an elliptical morphology, exhibiting a smooth, featureless appearance. Its shape is elongated, appearing cigar-shaped. The light distribution suggests a concentration of older stellar populations. The galaxy's color appears to be in the redder part of the spectrum, indicating lower ongoing star formation. There is no strong evidence of spiral arms, dust lanes, or active galactic nucleus activity based on the image. There is no visible evidence of a recent or ongoing major merger. The light is centrally concentrated, with a gradual decrease in intensity towards the outer regions.
