The galaxy presents as a somewhat rounded, centrally concentrated light distribution. The core region exhibits a bright, smooth morphology, transitioning to a less defined, more diffuse outer halo. There is evidence of a subtle disk-like structure surrounding the core, however, this structure is not sharply defined. No obvious spiral arms are visible. The galaxy appears relatively undisturbed, with only minor potential distortions, such as a slight asymmetry, suggesting the possibility of past or ongoing minor interactions. Overall, the galaxy appears to be a relatively massive system with a moderate rate of star formation. The color gradients suggest an older stellar population in the core, possibly transitioning to slightly younger populations in the outskirts.
