The galaxy appears as a singular, relatively smooth object. It exhibits a concentrated central bulge, transitioning into a more diffuse outer region. The galaxy displays a moderate yellow hue that suggests the dominance of older stellar populations. The object has an approximate effective radius of around 6 kpc. There appears to be little to no evidence of spiral arm structure or significant dust lanes. Indications suggest that the galaxy has a mass consistent with a large galaxy, exhibiting moderate levels of star formation. There does not appear to be any major ongoing merger or tidal disturbance.
