The galaxy presents as a generally smooth, rounded object with a concentrated central region. There is little evidence of spiral arm structure or a prominent disk. The core exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions appear more diffuse and exhibit a bluer tint, suggesting the presence of some younger stars or ongoing star formation, albeit at a low rate. The galaxy does not obviously appear to be undergoing any major merging activity or experiencing significant disturbances in its morphology. The overall impression is that of a relatively evolved system.
