The galaxy presents as a moderately sized object with a primarily smooth morphology. The light distribution appears centrally concentrated, fading gradually towards the outer regions. A slight elongation is observed, suggesting a non-spherical shape, perhaps tending towards a flattened, disk-like structure when considered three-dimensionally. A small amount of blue light is visible, suggesting the presence of at least some small amount of ongoing star formation, and it's observed to the side of the galaxy. Otherwise, the galaxy appears redder in overall color, hinting at a population of older, redder stars, in the center of the galaxy. There may be some evidence of a weak tidal interaction or disturbance given the asymmetry of the galaxy's light profile, although further investigation would be required to confirm such interactions.
