The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, featureless structure. It presents a generally rounded morphology, lacking a clearly defined spiral arm structure or distinct disk component. The central bulge is prominent, displaying a higher concentration of light intensity compared to the outer regions. The light distribution suggests a relatively old stellar population, with minimal evidence of ongoing active star formation within the galactic body itself. Faint tidal features or minor disturbances might be present but the galaxy seems largely undisturbed. It presents a soft blue hue in the center. The light is relatively uniform, suggesting a lack of significant dust lanes or patchy star formation regions within the galaxy itself.
