The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that dominates the overall light profile. The color appears generally yellow, with some suggestions of redder hues in the outer regions. There is a very faint hint of asymmetry. While the structure is predominantly smooth, the slight distortion could indicate a minor tidal interaction or recent merger event. Based on the color, we can infer that the galaxy hosts an older stellar population. The lack of well-defined spiral arms is consistent with a more quiescent star-forming environment.
