The galaxy presents as an elliptical form, with a smooth, diffuse light distribution, and a central bright region. The lack of distinct spiral arms or dust lanes suggests it is not a spiral galaxy, and it has been identified with a redshift of approximately 0.09, indicating its relative distance. Its overall color appears to be a slightly bluer hue, and its roundness indicates it lacks significant morphological disturbances. The lack of clear substructure within the galaxy suggests the possibility of an older stellar population within.