The galaxy presents an elliptical morphology, though with some visible irregularity. The light is concentrated in a relatively smooth central bulge, with a less well-defined and more diffuse halo. There is asymmetry in the light distribution, indicating a possible interaction or disturbance. One distinct region of bluer light is observed, possibly indicative of increased star formation activity relative to the rest of the galaxy. The overall color suggests an evolved stellar population, though the localized bluer region indicates the presence of younger stars. The object displays an intermediate apparent roundness, neither perfectly spherical nor highly elongated. There are visual indications of minor gravitational disturbance, though a significant portion of light is not obviously impacted by the gravitational disturbance.
