The galaxy appears as a relatively compact object, approximately circular in projection with a hint of ellipticity. It presents with a bright, concentrated central region or bulge that is possibly a galactic nucleus. The color profile suggests a redder core transitioning to bluer outer regions which indicates older stellar populations concentrated in the core, with younger, star-forming regions in the periphery. There are subtle indications of potential disturbances in the galaxy's morphology or possible tidal features suggestive of interactions with other galaxies. The overall impression suggests it is an older system, but with ongoing, albeit low, star formation in the outer areas.
