The galaxy presents as a roughly elliptical object, exhibiting a predominantly smooth morphology. The light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a lack of distinct spiral arm structures or prominent star-forming regions discernible within the image. The color is relatively uniform throughout the galaxy, suggesting an older stellar population. The image does not obviously present tidal features or disturbances which indicate a major merger event, though subtle asymmetries might be present. The object appears relatively isolated, with no immediately obvious signs of interaction with other galaxies. The galaxy appears moderately massive and has a low star-formation rate.
