The galaxy appears to be a luminous, elliptical system with a relatively smooth, centrally concentrated light distribution. There is a noticeable color gradient, with the core exhibiting a more yellowish-orange hue, transitioning to a slightly bluer tint in the outer regions. The galaxy exhibits a high degree of rotational symmetry, with minimal visible distortions or tidal features. There is no clear evidence of spiral arm structure or a prominent disk. Faint extensions around the core are visible in the low surface brightness region. The image is consistent with a relaxed system that does not show strong signs of recent merger activity, however, a small potential companion galaxy seems to be in very close proximity.
