The galaxy presents a predominantly elliptical morphology. It exhibits a smooth, centrally concentrated luminosity profile, indicative of an older stellar population. The overall color is slightly redder, supporting the hypothesis of diminished recent star formation. The light distribution appears relatively uniform and lacks any distinct spiral arm structures or prominent dust lanes. The galaxy is nearly circular with a relatively high Sersic index, suggesting it is a Sersic galaxy. There may be some tidal features or minor disturbances visible, but they are not obviously visible in this image.
