The galaxy presents a largely smooth, elliptical morphology. The light profile appears centrally concentrated with a relatively high degree of radial symmetry. There is no evidence of spiral arms or a prominent disk structure. The color is generally yellowish, suggesting a stellar population dominated by older, redder stars. There is a slight blue hue in a small section of the galaxy which may be from some recent star formation. There are no obvious signs of recent or ongoing major merger events, though there is the slight possibility of a minor disturbance given the irregular color profile. Overall, the galaxy appears to be a relatively evolved system, consistent with an elliptical classification.
