The galaxy presents as a slightly elongated, well-defined structure. A bright, concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population dominating the core. Surrounding the bulge, a more diffuse, bluish halo extends outwards, indicating the presence of younger, hotter stars and possibly ongoing star formation. The galaxy appears relatively smooth, with no prominent spiral arms or distinct dust lanes visible in this image. The overall shape leans toward elliptical, with a high degree of central concentration. There are hints of minor disturbances in the outer regions, but no clear indication of a major merger or interaction. The galaxy appears to be largely undisturbed.
