The galaxy presents as a relatively smooth, elliptical structure. Its light is dominated by warmer tones indicative of an older stellar population. There is a slight elongation visible, suggesting a deviation from a perfectly spherical shape, leaning towards a cigar-like structure. The morphology does not show any prominent signs of ongoing mergers or major disturbances; it appears mostly undisturbed. Overall, the galaxy appears to be a well-formed, quiescent system, with no intense star formation. 
