The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge or core. There appears to be a slight elongation or asymmetry along a single axis, suggesting a possible disk component viewed at a steep angle or a minor disturbance in its morphology. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to more subdued reddish hues in its outer regions. This may indicate older stellar populations dominating the outer areas and possibly ongoing, but comparatively low, star formation within the core. Overall, the galaxy appears to be an evolved system, with limited signs of active merging or significant morphological irregularities, though there's a slight hint of tidal interactions.
