The galaxy appears to be an elliptical or lenticular type, characterized by a centrally concentrated bulge. The core exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outward from the center, the galaxy displays a gradual decrease in brightness, transitioning to a more diffuse, bluish halo. The halo might show hints of a faint, disk-like structure, though it isn't clearly defined. The morphology is generally smooth and featureless, lacking distinct spiral arms or prominent dust lanes. There is no obvious sign of active galactic nuclei or starburst activity within the region. Overall, it shows a spheroidal shape and no distinct disturbances or mergers are visually apparent.
