The galaxy presents as a relatively smooth, centrally concentrated light distribution. The overall morphology appears to be elliptical or lenticular, with a high degree of roundness. There is little to no evidence of spiral arms or a distinct disk structure. The galaxy exhibits a color gradient, appearing bluer in the central region, which could indicate a population of younger stars, and becoming slightly redder towards the outskirts. There is no significant indication of tidal tails or other disturbances suggesting a recent major merger, though a subtle asymmetry might suggest minor interactions. Based on the color and smooth morphology, this galaxy is likely a relatively massive system with moderate levels of star formation.
