This galaxy appears to be a relatively smooth, elliptical galaxy. The light distribution is centrally concentrated, with a gradual decline in brightness towards the outer edges. The galaxy has a generally round shape, with no obvious disk features or spiral arms visible. There are no distinct signs of major disturbances, such as tidal tails or strong asymmetries, suggesting it is likely not undergoing a major merger. It has a redder color, suggesting an older stellar population and a lower rate of on-going star formation. There might be signs of a minor interaction.
