The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The central region exhibits a high concentration of light, indicative of a substantial bulge component. Color gradients suggest that the core is dominated by an older stellar population. The object appears to be isolated, without prominent signs of tidal interaction or recent mergers. There is a general lack of distinct spiral arms or prominent star-forming regions. The color suggests that this galaxy is well into the red sequence. 
