This galaxy appears to be a relatively smooth, luminous object with an elliptical morphology. It appears to be generally round in shape. There is a brighter central region, suggestive of a concentrated core or nucleus. The galaxy exhibits a redder color profile, possibly indicating an older stellar population. Based on its features and color, this is likely a massive galaxy with a reasonable amount of star formation, potentially in the process of merging with another galaxy. Some disturbance appears to be present, possibly from the aforementioned interaction with another galaxy.
