The galaxy presents as a centrally concentrated object with a diffuse and extended halo. The core exhibits a yellowish-white hue, suggesting an older stellar population. Fainter blue regions extend outwards from the central bulge, potentially indicating areas of more recent star formation, although the resolution is limited. There is a subtle asymmetry in the outer regions of the galaxy's disk and halo. There's no clear evidence of a spiral structure, and the overall morphology seems to lean towards a smoother, less defined shape. The galaxy does not show any prominent signs of tidal disturbances.
