The galaxy appears as a centrally concentrated, elliptical system. Its overall shape is elongated, with the major axis oriented vertically in this image. The light distribution suggests a relatively smooth profile, lacking prominent spiral arms or distinct features. The core region exhibits a strong concentration of light, appearing almost unresolved at this resolution. There is a noticeable color gradient, with the central region displaying a redder hue that transitions to a slightly bluer color towards the outer regions. This color variation could indicate an older stellar population concentrated at the center, with a younger, star-forming population residing in the outskirts. There is no apparent sign of any active galactic nuclei or recent merger events. However, there is a faint, asymmetric extension or tidal feature may be present to the left.
