The galaxy appears as a centrally concentrated object, with a relatively smooth, elliptical morphology. A slight elongation is noticeable, suggesting it is not perfectly spherical. The color distribution indicates a predominantly older stellar population, with a central reddish hue possibly indicating a concentration of evolved stars. There's some evidence of bluer components in the outer regions, which may indicate more recent star formation activity at the outskirts. No prominent spiral arms or distinct features are apparent, suggesting it is likely an early-type galaxy. There is a slight disturbance which could be signs of a minor interaction.
