The galaxy presents as a centrally concentrated object with a diffuse, spheroidal morphology. The core region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. Moving outwards from the center, the light becomes fainter and more diffuse, exhibiting a transition in color towards a slightly redder tone. This may indicate the presence of an aging stellar population in the outer regions of the galaxy. There are no apparent spiral arm structures or prominent dust lanes visible in this image. The overall smoothness of the light distribution suggests a relatively relaxed morphology, characteristic of elliptical or lenticular galaxies. Subtle irregularities in the outer regions could potentially indicate minor disturbances or interactions, however this is difficult to confirm without additional data.
