The galaxy appears as a relatively compact object with a dominant central bulge. There's a slight asymmetry in the light distribution, which might indicate a minor tidal disturbance or interaction, although a clear merging signature is not readily apparent. The galaxy exhibits a relatively smooth light profile, with a general lack of distinct spiral arm structures, consistent with an elliptical morphology or a lenticular galaxy seen at a shallow inclination angle. It presents a blue-ish hue suggesting a moderate degree of ongoing star formation activity.
