The galaxy presents a largely smooth, elliptical morphology, appearing relatively round. The light distribution is concentrated towards the center, exhibiting a bright, distinct core. Fainter, diffuse light extends outwards from the core, diminishing with radial distance. There is no readily apparent spiral structure, dust lanes, or prominent star-forming regions visible. The color profile appears broadly consistent, with the inner regions perhaps exhibiting a slightly yellower hue, which could indicate an older stellar population or increased dust content relative to the outer regions, though the outer edges also contain yellow light. No strong evidence of recent merger activity or tidal distortions are observed. The overall impression is that of a fairly evolved, quiescent system.
