The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a concentrated central bulge. It appears somewhat round in shape. There are no immediately obvious signs of spiral arm structure or a prominent disk. Color gradients are present, with a yellowish-white core gradually fading into a slightly redder halo. There are only minor signs of any disturbances to its structure, indicating that it is likely a relatively isolated system or one that has completed the bulk of any recent merger activity. The estimated physical size of the galaxy is around 5.5 kpc. Although, the galaxy is fairly faint, it is estimated to be relatively large and massive. Star formation is present, but it appears relatively low.
