The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is visually dominant. There appears to be a slight elongation to the structure, deviating from a perfectly circular shape. Color gradients are subtle, with a slightly more yellow hue concentrated towards the core, suggesting an older stellar population in that region. There is a faint, diffuse halo extending outwards, but no prominent spiral arms or dust lanes are discernible within this image. There is no indication of tidal tails or morphological disturbances that might indicate ongoing or recent merger activity. The overall appearance suggests a relatively quiescent and evolved system.
