This galaxy exhibits a largely smooth, elliptical morphology, appearing somewhat rounded in shape. The primary light distribution suggests a high degree of central concentration, characteristic of early-type galaxies. There is a subtle color gradient, with the central region appearing bluer, potentially indicating a small amount of ongoing star formation or a younger stellar population relative to the galaxy's outer regions. A secondary, more compact redder source is seen near the main galaxy, and appears to be related to an area of disturbance. This could indicate a minor interaction or tidal effect due to the presence of a companion galaxy, which appears very close in angular separation. There is no clear evidence of spiral arm structure or a prominent disk component.
