The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution. The core is highly luminous, appearing a concentrated yellow-white. Moving outward from the core, the luminosity decreases, with a discernible but faint halo extending in all directions. There may be very faint hints of possible spiral arm structure, but they are not well defined. The color gradient suggests the presence of an older stellar population. The isophotes exhibit a general elliptical shape but appear slightly flattened and elongated. No obvious signs of tidal disturbances or ongoing mergers are apparent.
