The galaxy presents as a somewhat diffuse, elliptical-like structure with a smooth appearance. Its core exhibits a bright, concentrated luminosity, suggesting a significant density of stars or the potential presence of an active galactic nucleus, though this cannot be definitively confirmed from the image alone. The radial color profile appears slightly redder in the central region, shifting to a bluer hue in the outer edges. There is little evidence of spiral arms or distinct disk features. The galaxy displays a moderate size relative to other galaxies in its vicinity and appears relatively isolated, showing no significant signs of tidal disruption or ongoing major merger activity. Overall, it seems to be an elliptical galaxy with a relatively high degree of smoothness.
