The galaxy presents as a single, moderately bright object. It exhibits a somewhat smooth, disk-like morphology, although some features are visible suggesting internal structure. A subtle central bulge is apparent, surrounded by a more diffuse halo. The color profile indicates a potential mix of stellar populations, trending towards redder hues in the central region and bluer tones in the outer regions. The overall roundness suggests a possible classification as an early-type spiral or a lenticular galaxy. There is a slight hint of disturbance in the galaxy's form, it could indicate a minor interaction or merging event.
