The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth morphology with a slight elongation. The central bulge is prominent and displays a concentrated, yellowish-white hue, suggesting an older stellar population. The outer regions show a gradual decrease in brightness, fading into a more diffuse disk-like structure with a slightly bluer tint. There is no evidence of significant spiral arms, large dust lanes, or ongoing major mergers, although a faint, irregular feature might suggest a minor disturbance or interaction. Overall, it appears to be a massive galaxy undergoing relatively low levels of star formation, with a dominant population of evolved stars.
