The galaxy appears to be an elliptical or lenticular type, with a predominantly smooth morphology. There is a concentration of luminosity towards the center. The galaxy exhibits a near spherical shape but seems slightly more elliptical. No distinct spiral arms or bar structures are discernible. There is a relatively small star formation rate, and very high specific star formation rate. There is no major merging apparent, but there is a very slight minor disturbance in the galaxy's smooth structure. It's magnitude appears to be around 18-20. The estimated size of the galaxy is a little less than 3 kpc.
