The galaxy presents a generally smooth morphology, appearing largely featureless. It exhibits an elliptical shape with a high degree of roundness. The central region displays a strong concentration of light, suggesting a significant stellar population and/or an active galactic nucleus. A faint, diffuse halo surrounds the core, gradually fading into the background. There are hints of subtle disturbances in the outer regions, potentially indicating past interactions, but no obvious major mergers or tidal tails are immediately apparent. Colors suggest the presence of both older stellar populations and a component of ongoing, though perhaps subdued, star formation. Overall, the galaxy appears to be a massive system, with a considerable luminosity.
