The galaxy appears as a moderately elongated, diffuse object with a relatively smooth texture. It exhibits a central concentration of light, suggesting a bulge or core region. There is a slight color gradient, with the central region appearing somewhat bluer than the outer edges. This color difference could indicate differences in stellar populations, with the bluer core potentially indicating ongoing or recent star formation. There are no prominent spiral arms or distinct morphological features readily apparent. The overall appearance is suggestive of an early-type galaxy, possibly an elliptical or lenticular system, but the slight elongation could also indicate a disk component viewed at a shallow angle. There seems to be a slight disturbance and a potential hint of an interaction or merger.
