The galaxy appears as a centrally concentrated object, exhibiting a smooth light distribution. The core region is relatively bright, with a gradual decrease in luminosity extending outwards. There is little evidence of spiral arm structure or distinct star-forming regions. A faint, extended halo may be present, but this is difficult to ascertain. The shape is generally round. There is no strong evidence of ongoing major merger activity, although a subtle asymmetry could indicate a minor interaction or disturbance. The galaxy's overall color suggests a relatively evolved stellar population, though a small region of bluer stars hints at modest levels of recent star formation.
