The galaxy presents a morphology consistent with an elliptical or lenticular type, displaying a generally smooth light distribution. The main body appears relatively spherical. A small disturbance can be seen on the edge of the galaxy, indicating a possible minor interaction with a companion galaxy, or residual effects from a previous merger. The color profile appears largely homogenous, skewed toward the red end of the spectrum, with an intense core, suggestive of an older stellar population and reduced star formation activity. This galaxy is a rather massive example of its type.
