The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Color gradients are subtle, with a generally reddish-orange hue dominating. There is minimal visual evidence of distinct spiral arms or active star-forming regions, suggesting an older stellar population. The galaxy appears slightly elongated, with no major disturbances or signs of ongoing merging events visible. Overall, it seems to be a massive galaxy undergoing low levels of star formation.
