The galaxy presents as a single, concentrated luminous object. Its morphology is overwhelmingly smooth and rounded. A slight elongation is barely perceptible. The color profile is dominated by redder wavelengths in the core, transitioning to a slightly bluer halo. No clear spiral arm structures or distinct features are visible, suggesting a spheroid-dominated morphology. The object is generally isolated, without any strong indications of ongoing major mergers or tidal disturbances. Based on the observed characteristics, the galaxy appears to be a relatively quiescent system, likely of significant mass and with very minimal star formation.
