The galaxy appears to be a relatively smooth, elliptical-like system, with a concentrated central bulge region exhibiting a yellow-orange hue, suggesting an older stellar population. The galaxy shows a moderate ellipticity, appearing elongated rather than perfectly spherical. There is an indication of a possible faint, diffuse disk component or tidal feature at the bottom of the image, showing some green emissions suggesting ongoing star formation in this region. There is no clear evidence of spiral arm structure or a prominent dust lane. Overall, the galaxy exhibits characteristics of a system undergoing, or has undergone, significant aging of its stellar population.
