The galaxy presents an elliptical morphology, appearing largely smooth with a high degree of central concentration of light. The overall shape suggests a spheroid with an observed flattening. There's a gradual decrease in luminosity from the core to the outer edges. The color profile is relatively uniform, indicating a lack of significant star forming regions, and a stellar population possibly dominated by older, redder stars. There is a possible slight warp. There is no presence of spiral arms or distinct dust lanes visible in the image. The galaxy appears relatively isolated. 
