The galaxy presents as a relatively smooth, elliptical structure with a distinct central bulge. There is no clear evidence of spiral arms or a prominent disk. The light distribution suggests a high degree of spherical symmetry. The galaxy appears compact, and it exhibits a concentration of light intensity towards its core. Color gradients are subtle, with a possible slight bluer hue towards the outer regions, but overall, the galaxy appears to have a redder color profile, indicative of an older stellar population. There is no indication of active star formation regions or strong dust lanes visible in this image. Based on the observed morphology, this is likely a relatively massive, evolved galaxy.
