The galaxy presents a largely smooth, elliptical morphology. It is observed to have a centrally concentrated bulge region exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. Extending outwards from the central bulge is a fainter, more diffuse halo or envelope of light. This outer region appears less structured and more uniform in color distribution, with subtle hints of bluer tones within the yellow. There is no discernible spiral arm structure nor any indications of active star formation regions like HII regions. The overall shape is closer to intermediate between round and elongated, suggesting it is not perfectly spherical but neither significantly flattened. There are no clear signs of interaction or merging events in this image.
