The galaxy presents as a relatively smooth, elliptical-like structure, appearing somewhat elongated but without a clearly defined disk. It exhibits a strong central bulge that dominates the galaxy's luminosity profile. The color gradient suggests an older stellar population in the central regions, shifting towards bluer hues in the outskirts. There is no clear evidence of active star formation regions or prominent dust lanes. Overall, the galaxy's morphology suggests a classification as an early-type galaxy, likely an elliptical or lenticular, with little ongoing merger activity or major disturbances. 
