The galaxy exhibits a generally smooth morphology, with a distinct elliptical shape, appearing cigar-shaped. The light distribution shows a central concentration, with the brightest region occupying the core, fading gradually outward. Color gradients are subtle, with the central region appearing somewhat yellower, suggesting an older stellar population, while the outer regions have a bluer tinge, potentially indicating the presence of younger, hotter stars, though star formation appears minimal overall. There is no visible evidence of spiral arms or a prominent disk structure. No significant tidal features or signs of recent major merger activity are apparent. The overall structure indicates a relatively evolved system.
