The galaxy presents a largely smooth morphology, with a slight deviation from perfect ellipticity. The central region exhibits a pronounced brightness, suggesting a concentrated nucleus. Surrounding the core is a less luminous, extended halo, exhibiting a subtle blue-green hue. There is very little visual evidence of spiral arm structures or dust lanes. The outer edges appear to gradually fade into the background, indicating a smooth density profile. Minor irregularities are observable in the halo, indicating a possible interaction or merger event. The system appears relatively isolated, showing no large interacting companion galaxies within the immediate vicinity.
