The galaxy presents as a centrally concentrated object with a diffuse, extended halo. Its light profile suggests a relatively smooth, featureless structure, with no apparent spiral arms or bar. The core exhibits a yellowish hue, potentially indicating an older stellar population. The galaxy's overall shape appears somewhat elliptical, tending towards being 'in between' round and cigar-shaped. There is no visible evidence of a major ongoing merger, though minor distortions cannot be ruled out at this resolution.
