The galaxy presents a generally smooth, elliptical morphology with a slight elongation. A dominant central bulge is visible, exhibiting a concentrated, bright yellowish-orange hue. This likely signifies an older stellar population. Fainter, extended regions of diffuse light surround the bulge, appearing slightly bluer and more uneven. These regions may indicate ongoing, albeit limited, star formation. There is a faint hint of a disk, or perhaps some disturbance in the galaxy's structure, with some asymmetrical distribution of light in the outer regions. Overall the galaxy appears to be a massive galaxy exhibiting low star formation. There is evidence of a potential interaction or merger event due to the disturbed morphology and asymmetrical features.
