The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular classification. Its overall shape approximates a rounded form, exhibiting minimal deviation from circular symmetry. While a central concentration of light is evident, the galaxy lacks any prominent spiral arms or other distinct features indicative of active star formation within a disk structure. There are no obvious signs of recent merger events or significant tidal disturbances influencing its structure. The color distribution appears relatively uniform, with a slight bluer tint toward the center which hints at some ongoing, though likely subdued, star formation. The galaxy is relatively compact, with a moderate angular size on the image plane.
