The galaxy presents a largely smooth morphology, exhibiting a concentrated, rounded structure. The central region displays a yellowish-white hue, suggesting a population of older stars. The color profile transitions subtly outwards, becoming slightly redder in the outer regions. There is no obvious presence of spiral arms or a prominent disk. The overall appearance implies an elliptical galaxy with minimal recent star formation activity. Subtle irregularities in the outer profile possibly hint at minor past interactions, although no distinct tidal features or ongoing merger events are apparent. The relative lack of blue light suggests a low specific star formation rate.
