The galaxy presents a generally smooth and elliptical morphology. It appears to be relatively quiescent, showing no distinct spiral arms or active star-forming regions discernible in the image. There is a slightly elongated shape, though it mostly appears round. The central region is brighter and yellowish, suggesting a higher concentration of older stars. The outer regions are dimmer and may have a bluer hue, potentially indicating some amount of younger stellar populations. Overall, the galaxy appears to be a relatively massive, evolved system. There is a very slight possibility of a minor disturbance on the upper left side, but it could be an artifact. There is no evidence of significant ongoing merger activity or major disturbances in the image.
