The galaxy presents as a single, relatively smooth object with a slightly elliptical morphology. The light distribution appears centrally concentrated with no obvious spiral arm structures or prominent star-forming regions readily discernible in the image. The color profile suggests a somewhat redder overall population, consistent with a galaxy dominated by older stellar populations and a low rate of current star formation. There's a hint of a more diffuse, extended halo surrounding the central region. Close inspection does not reveal evidence of ongoing major merger activity, although subtle distortions or minor irregularities within the main body could potentially indicate past interactions or minor disturbances. The galaxy is not perfectly round but appears somewhere between round and cigar shaped.
