The galaxy presents a predominantly smooth morphology with a central bulge that appears roughly circular. A subtle disk-like feature is possibly present, though not sharply defined. The color profile suggests a relatively mature stellar population, with a redder hue concentrated in the central regions and a slight shift towards bluer tones in the outer regions. There are indications of possible disturbances or tidal features, which would imply an interaction with another galaxy. However, there is no strong evidence for a major ongoing merger.
