The galaxy presents a generally elliptical morphology, appearing significantly more elongated than circular. The light distribution is centrally concentrated, with a bright, somewhat diffuse core exhibiting a yellowish hue. Surrounding the core is an extended envelope of fainter material, also displaying a yellowish tint. There are no prominent spiral arms or distinct dust lanes visible in the image. Based on the galaxy's smooth appearance, it is likely a relatively massive galaxy. The overall color suggests an older stellar population with a low rate of star formation. There is a subtle suggestion of a possible minor disturbance in the outer regions, but it is not substantial. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger event.
