The galaxy appears to be a generally smooth, centrally concentrated object with a round morphology. The core of the galaxy exhibits a bright, yellowish-white hue, suggesting an older stellar population or potentially significant dust obscuration. Moving outwards from the core, the galaxy transitions to a fainter, reddish-orange color. The outer regions are diffuse and lack distinct structural features such as spiral arms or a prominent disk. There is no clear evidence of a recent major merger or strong tidal interactions, although subtle disturbances or minor companions may exist but are not discernible at this resolution. The overall appearance suggests a relatively evolved system, possibly an elliptical or lenticular galaxy.
