The galaxy appears to be a relatively smooth, elliptical or lenticular type. It has a centrally concentrated luminosity profile, with a bright, reddish core indicative of an older stellar population. Surrounding the core is a more diffuse, bluish halo. The overall shape is largely spheroidal, appearing fairly round and without any prominent spiral arms or bar structures. There is no obvious evidence of recent major merger events. Subtle colour gradients may indicate variations in stellar populations or dust content within the galaxy. The galaxy is of intermediate size, neither a dwarf nor a giant. Star formation rate appears low, with possible recent star formation in the extended halo. The morphology suggests the galaxy is relatively evolved.
