The galaxy appears as a single, mostly uniform object with a concentrated central region. The light profile suggests a relatively smooth distribution, lacking prominent spiral arms or irregular features that would suggest a more complex morphology. The shape is predominantly round. There is a slight color gradient, shifting from yellower hues in the central core to marginally redder tones in the outer regions. This could indicate variations in stellar populations, with older, redder stars potentially dominating the outskirts. The overall color profile suggests relatively low star formation. There is no indication of tidal disturbances or ongoing mergers.
